Constellation Aquila (Eagle)

Properties
Aquila is one of the summer constellations. Its brightest star, Atair, marks the well-known summer triangle with Deneb (α Cygni) and Vega (α Lyrae). Sagitta. The star Atair can be easily recognized by its two weaker companions (β and γ Aquilae), who accompany it like bodyguards on the right and left; they are named Alshain and Tarazed, both of which are derived from the Persian name of the constellation, Shahin tara zed (star-studded falcon). This formation is the most striking feature of this constellation, which contains star-rich areas, especially near the southwestern border with Scutum. The area of Aquila is 652 square degrees and it culminates at midnight on around July 12th. [9, 15]
Stars with Proper Names:
- α Aql: Altair, Atair
- β Aql: Alshain, Alschairn
- γ Aql: Tarazed, Reda
- ε Aql: Deneb El Okab, Deneb
- ζ Aql: Deneb El Okab, Deneb
Deep-Sky Object Descriptions
Mythology and History
A constellation from ancient times. It had been known as the Adler for over 3000 years. In Greek mythology, the eagle stole Antinous, one of the suitors of Penelope, the wife of Odysseus, and brought him to Olympus, where he became a servant of the gods. The eagle was always at Zeus' side in his long battle against the titans for control of the universe. His job was to carry Zeus' thunder arrows so that he could use them to kill the titans. [73]

Aquila also played a role in domestic affairs on Mount Olympus, the seat of the gods. One day the gods needed a new cup carrier to serve them fresh nectar. But this task could only be done by the most beautiful youth on earth. The eagle was sent out to find a new cup-bearer. When he brought the stately Trojan prince Ganymedes to Zeus, the king of the gods was so delighted that he gave the eagle a place under the stars. [73]
An eagle also appears in the Hercules legend. On the way to the tree with the golden apples of eternal youth on the western edge of the earth, Hercules passed a lonely place in the Caucasus. Prometheus, a son of the sky god Uranus and mother earth, lay there forged on a rock. This was the punishment of the gods, since Prometheus created people out of clay for whom he is said to have later stolen the fire from heaven. An eagle came by every day, tore open its body with its pointed, crooked beak and ate at its liver. When Hercules saw this gruesome spectacle, he shot the eagle with an arrow and thus freed Prometheus - at least for a short time - from his torment. An arrow still flies over the constellation Aquila today - did Hercules not hit it after all? [20]
Another version of the first episode is followed by the name The Eagle with the Antinous or Servans Antinoum: The favorite boy of Emperor Hadrian (2nd century AD), an ideal of youthful beauty, was drowned in a river, it is not known whether it was an accident or he drowned himself in order to obtain a long life for his patron Hadrian through this sacrificial death. Shortly afterwards Zeus sent his eagle to lift Antinous up to the starry sky. Many star maps show the boy in the clutches of the eagle and for some time he was listed as a separate constellation south of Aquila. [20, 62]
Catalogs
HR | B | F | DM | HD | SAO | FK5 | IR | M* | ADS | VarID | RA | Dec | vMag | spType | dMag | Sep ["] | Remarks |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
HR 7040 | 4 | BD+01 3766 | 173370 | 123879 | 11290 | 18 44 49.9 | +02 03 36 | 5.02 | B9V e | S:Shell star. H alpha emission.,VAR:Gamma Cas?, 5.00 - 5.05V. | |||||||
HR 7059 | 5 | BD-01 3559 | 173654 | 142606 | 11667 | 18 46 28.5 | -00 57 42 | 5.90 | A2Vm | 1.6 | 12.8 | D:AB binary, B, Am, F3Vm, or Am(A5/F1/F2), RV +9.2k/s, vsini =<25k/s. C, 11.3v optical.,G:Sirius group; UMa stream.,S:Also classified Am(A1/A7V/A7).,SB:ADS 11667A, spectrum binary, RV var.? Unresolved by speckle interferometry on 1976.30; companion with sep. 0.13" seen,SB:on 1980.48 (McAlister and Hartkopf). | |||||
HR 7085 | BD+00 4027 | 174240 | 123947 | 18 49 37.1 | +00 50 09 | 6.25 | A1V | ||||||||||
HR 7099 | BD+10 3685 | 174569 | 104170 | I | 11750 | 18 50 45.6 | +10 58 35 | 6.55 R | K5III+K3III | 1.1 | 3.5 | D:Binary, companion K3III-IV. | |||||
HR 7101 | 8 | BD-03 4392 | 174589 | 142706 | 3500 | 18 51 22.1 | -03 19 04 | 6.10 | F2III | ||||||||
HR 7135 | BD+06 3978 | 175515 | 124050 | 3509 | I | 11536 | 18 55 27.5 | +06 36 55 | 5.57 | K0III | SB:2994d, K 4.65k/s, V0 +23.31k/s, asini 186. | ||||||
HR 7143 | BD-01 3602 | 175640 | 142825 | 3510 | 18 56 22.7 | -01 48 00 | 6.22 | B9III | S:HgMn star. | ||||||||
HR 7163 | BD+06 3989 | 176095 | 124112 | 18 58 23.8 | +06 14 25 | 6.21 | F5IV | ||||||||||
HR 7165 | BD+17 3799 | 176155 | 104296 | 11884 | FF Aql | 18 58 14.7 | +17 21 39 | 5.38 | F8Ib | 5.3 | 6.6 | D:Companion blue star?,SB:1435d, K 3.5k/s, V0 -17.4k/s, asini 69.1. RV may also vary in 4109d.,VAR:ADS 11884A, CDelta 5.18 - 5.68V, 4.470916d. Magnetic field. Possible blue companion. | |||||
HR 7167 | 10 | BD+13 3838 | 176232 | 104303 | V1286 Aql | 18 58 46.9 | +13 54 24 | 5.89 | F0pSrEu | G:Sirius group?,S:Oxygen deficient relative to magnesium. Magnetic star. Also classified A4p.,VAR:Alpha CV 5.83 - 5.93V. Published periods of 6.05 and 9.78d probably spurious; nor does a more recent 6.5386d satisfy,VAR:all observations. Period may be years. Abt and Golson found range 5.83 - 5.91V. Two isolated obs. of 5.93 and 5.94V,,VAR:while other observers report intermediate values with amp. <0.015V. | |||||||
HR 7172 | 11 | BD+13 3841 | 176303 | 104308 | 11902 | 11618 | 18 59 05.7 | +13 37 21 | 5.23 | F8V | 4.3 | 17.8 | D:Both companions optical.,G:UMa stream. | ||||
HR 7173 | BD+09 3951 | 176304 | 104313 | 18 59 17.5 | +10 08 27 | 6.75 | B2Vp | ||||||||||
HR 7176 | ε | 13 | BD+14 3736 | 176411 | 104318 | 712 | I | W | 18 59 37.4 | +15 04 06 | 4.02 | K1-IIICN0.5Ba0.2 | 5.9 | 131.1 | C:V magnitudes scatter from 5.56 to 5.81, B-V from +0.35 to +0.45, U-B from -0.01 to +0.04.,N:Deneb el Okab; Deneb. Names combined with HR 7235. | ||
HR 7193 | 12 | BD-05 4840 | 176678 | 142931 | I | 11655 | 19 01 40.8 | -05 44 20 | 4.02 | K1III v | |||||||
HR 7208 | BD+08 3951 | 176981 | 124184 | 19 02 21.6 | +08 22 27 | 6.30 | K2III | ||||||||||
HR 7209 | 14 | BD-03 4460 | 176984 | 142959 | W | 19 02 54.5 | -03 41 56 | 5.42 | A1V | 0.0 | 0.1 | D:Sep. 0.099". Consistently unresolved by speckle observations at five epochs between 1977.48 and 1981.47 (McAlister,D:and Hartkopf).,G:Hyades group. | |||||
HR 7214 | BD+01 3865 | 177178 | 124203 | 19 03 32.2 | +01 49 08 | 5.83 | A4V | ||||||||||
HR 7219 | BD+03 3882 | 177332 | 124219 | 19 04 10.7 | +03 19 50 | 6.73 | A5m | ||||||||||
HR 7220 | BD-05 4858 | 177336 | 142985 | I | V Aql | 19 04 24.2 | -05 41 06 | 6.90 | C5II | VAR:SRb 6.6 - 8.4v, 10.6 - >12.4p, 353d. Mean mag. varies in cycle of about 2270d. | |||||||
HR 7225 | 15 | BD-04 4684 | 177463 | 142996 | I | 12007 A | 19 04 57.6 | -04 01 53 | 5.42 | K1III | 1.6 | 38.5 | D:Companion gK4, optical. | ||||
HR 7231 | BD-01 3642 | 177552 | 143003 | 19 05 18.6 | -01 30 46 | 6.53 | F1V | ||||||||||
HR 7235 | ζ | 17 | BD+13 3899 | 177724 | 104461 | 716 | I | 12026 | 11724 | 19 05 24.6 | +13 51 48 | 2.99 | A0Vn | 8.4 | 158.6 | DYN:0.020".,G:Pleiades group.,N:Deneb el Okab; Deneb. Combined with HR 7176. | |
HR 7236 | λ | 16 | BD-05 4876 | 177756 | 143021 | 717 | I | 19 06 14.9 | -04 52 57 | 3.44 | B9Vn | ||||||
HR 7243 | BD+08 3970 | 177940 | 124266 | I | W | R Aql | 19 06 22.2 | +08 13 48 | 6.09 | M7IIIe v | 5.0 | 180.7 | S:OH and H2O emission. IR spectra show water vapor. OH, H2O and SiO maser. Also classified M5e-M9e.,VAR:M 5.5 - 12.0v, 284.2d. Period changes 348.980 - 0.554202n + 0.000552309n2 from JD 2399190. Radio flare detected,VAR:in this position. | ||||
HR 7245 | BD+00 4106 | 178065 | 124282 | 19 07 09.1 | +00 38 30 | 6.56 | B9III | RV:Period 6.87d.,S:HgMn star. | |||||||||
HR 7248 | 18 | BD+10 3787 | 178125 | 104488 | 3525 | Y Aql | 19 06 58.6 | +11 04 17 | 5.09 | B8III | G:Possible Pleiades group.,SB:1.3023d, K 27.6k/s, V0 -18.7k/s, asini 0.494.,VAR:E 5.02 - 5.06B, 1.30227d. Form of light curve possibly variable. | ||||||
HR 7266 | 19 | BD+05 4040 | 178596 | 124318 | 3530 | 19 08 59.9 | +06 04 24 | 5.22 | F0III-IV | ||||||||
HR 7269 | BD-00 3662 | 178744 | 143087 | 19 09 51.6 | -00 25 41 | 6.34 | B5Vn | ||||||||||
HR 7279 | 20 | BD-08 4887 | 179406 | 143134 | 1500 | 11808 | 19 12 40.7 | -07 56 22 | 5.34 | B3V | |||||||
HR 7287 | 21 | BD+02 3824 | 179761 | 124408 | 3537 | 12182 | V1288 Aql | 19 13 42.7 | +02 17 37 | 5.15 | B8II-III | 7.5 | 36.2 | D:Companion optical.,VAR:Alpha CV 5.06 - 5.16V, 1.73d. | |||
HR 7288 | BD+05 4081 | 179791 | 124410 | 11827 | 19 13 44.1 | +05 30 57 | 6.49 | A2Vp | S:Lambda Boo star, Mg 4481 wk. | ||||||||
HR 7300 | BD+14 3846 | 180262 | 104655 | W | 19 15 20.1 | +15 05 01 | 5.57 | G8II-III | 2.1 | 89.6 | D:Binary. Companion A1V. | ||||||
HR 7303 | 22 | BD+04 4045 | 180482 | 124455 | 19 16 31.0 | +04 50 05 | 5.59 | A3IV | |||||||||
HR 7307 | BD+14 3852 | 180555 | 104668 | 12248 | 19 16 26.8 | +14 32 41 | 5.63 | B9.5V | 3.8 | 8.2 | D:AB CPM, B is 9.07V, +0.14(B-V), -0.05(U-B), F8V or G0IV, optical? Speckle interferometry indicates a fourth companion,D:at 0.051" from A. | ||||||
HR 7313 | BD+01 3960 | 180782 | 124478 | 19 17 48.2 | +02 01 54 | 6.19 | A1Vn | S:High velocity metal-rich subgiant. | |||||||||
HR 7315 | ω1 | 25 | BD+11 3790 | 180868 | 104691 | 725 | 19 17 49.0 | +11 35 43 | 5.28 | F0IV | |||||||
HR 7319 | 23 | BD+00 4168 | 180972 | 124487 | I | 12289 | 11889 | 19 18 32.5 | +01 05 07 | 5.10 | K2II-III v | 4.1 | 3.1 | D:AB binary. C, 13.7v at 12" optical.,DYN:0.004". | |||
HR 7321 | 24 | BD+00 4170 | 181053 | 124492 | W | 19 18 50.9 | +00 20 21 | 6.41 | K0-IIIa:Ba0.4CH1 | 0.2 | 423.4 | ||||||
HR 7325 | BD+09 4057 | 181122 | 124497 | 19 18 52.7 | +09 37 05 | 6.32 | G9III | G:Wolf 630 group. | |||||||||
HR 7331 | 28 | BD+12 3879 | 181333 | 104722 | W | V1208 Aql | 19 19 39.3 | +12 22 29 | 5.53 | F0III | 3.5 | 60.2 | VAR:Delta Sct 5.51 - 5.57V. Period analyses of new and existing data by Reed and Welch (1988, AJ, 95, 1510) indicate a,VAR:possible change in pulsational modes during the last several years, with fundamental period of 0.146d and possible,VAR:nonradial pulsations of 0.141, 0.183, and 0.091d. | ||||
HR 7332 | ω2 | 29 | BD+11 3802 | 181383 | 104728 | 19 19 53.0 | +11 32 06 | 6.02 | A2V | ||||||||
HR 7333 | 26 | BD-05 4936 | 181391 | 143286 | 3544 | I | W | 19 20 32.9 | -05 24 57 | 5.01 | G8III-IV | 6.8 | 115.9 | D:B probably optical.,M:Possible X-ray source 3U1915-05.,SB:266.544d, K 29.9k/s, V0 -18.0k/s, asini 61.1. High orbital eccentricity, 0.83. | |||
HR 7336 | 27 | BD-01 3716 | 181440 | 143292 | 19 20 35.7 | -00 53 32 | 5.49 | B9III | |||||||||
HR 7347 | BD-08 4950 | 181858 | 143321 | 19 22 20.7 | -08 12 04 | 6.31 | B3IVp | ||||||||||
HR 7349 | BD-00 3725 | 181907 | 143324 | 3546 | 19 22 21.5 | -00 15 09 | 5.83 | gG8 | |||||||||
HR 7353 | BD-07 4942 | 182038 | 143340 | I | 19 23 04.6 | -07 24 01 | 6.32 | K0 | |||||||||
HR 7354 | BD+09 4081 | 182101 | 124564 | 3548 | 19 22 48.4 | +09 54 47 | 6.35 | F6V | |||||||||
HR 7357 | BD+14 3896 | 182239 | 104779 | 19 23 08.2 | +14 55 16 | 6.64 | F1V | ||||||||||
HR 7366 | BD-05 4964 | 182475 | 143373 | 19 25 01.6 | -04 53 03 | 6.52 | A9V | ||||||||||
HR 7373 | 31 | BD+11 3833 | 182572 | 104807 | 1503 | W | 11994 | 19 24 58.2 | +11 56 40 | 5.16 | G8IVHdel 1 | 3.5 | 105.6 | D:Unresolved by speckle interferometry 1986.46.,G:61 Cyg group. | |||
HR 7377 | δ | 30 | BD+02 3879 | 182640 | 124603 | 730 | I | W | 12004 | 19 25 29.9 | +03 06 53 | 3.36 | F3IV | 7.5 | 108.9 | D:Component A astrometric binary, A* 3.36 F0IV, 3.422y, a = 0.058"; unresolved by speckle interferometry.,SB:0.1571d.,VAR:Delta Sct? Proper motion slightly variable? | |
HR 7387 | ν | 32 | BD+00 4206 | 182835 | 124628 | I | W | 12021 | 19 26 31.1 | +00 20 19 | 4.66 | F2Ib | 4.2 | 201.0 | C:V magnitudes scatter from 4.64 to 4.72, B-V from +0.58 to +0.61, U-B from +0.33 to +0.59.,D:Colors of B are +0.31(B-V), +0.16(U-B). | ||
HR 7389 | BD+12 3907 | 182900 | 104832 | 19 26 24.1 | +13 01 26 | 5.74 | F6III | G:Hyades group.,S:Also classified F7IV and F6V. | |||||||||
HR 7396 | BD+13 4020 | 183144 | 104862 | 3555 | 12049 | 19 27 33.9 | +14 16 57 | 6.32 | B4III | ||||||||
HR 7397 | BD+02 3892 | 183227 | 124661 | 19 28 20.8 | +02 55 49 | 5.85 | B6III | ||||||||||
HR 7400 | 35 | BD+01 4010 | 183324 | 124675 | 19 29 01.0 | +01 57 01 | 5.80 | A0IVp | G:In Ursa cluster?,S:Lambda Boo star, Mg 4481, met. wk. | ||||||||
HR 7402 | BD-07 4968 | 183344 | 143454 | 12503 | U Aql | 19 29 21.5 | -07 02 38 | 6.61 | F7-G1I-II v | 5.5 | 1.5 | D:AB fixed. C, 7v at 2", binary.,S:Also classified F5I-II-G1.,VAR:ADS 12503A, CDelta 6.08 - 6.86V, 7.02393d. Period changes. | |||||
HR 7404 | BD-00 3760 | 183387 | 124681 | I | 19 29 18.0 | +00 14 46 | 6.25 | K2 | |||||||||
HR 7407 | BD+14 3936 | 183492 | 104896 | 19 29 22.1 | +14 35 45 | 5.56 | K0III | ||||||||||
HR 7412 | BD+02 3904 | 183589 | 124698 | I | 12520 | 12088 | 19 30 10.5 | +02 54 15 | 6.09 | K5Ib | 4.9 | 34.1 | D:B, optical. | ||||
HR 7414 | 36 | BD-03 4612 | 183630 | 143482 | 1509 | I | 12093 | 19 30 39.8 | -02 47 20 | 5.03 | M1III v | ||||||
HR 7415 | BD+03 4043 | 183656 | 124704 | V923 Aql | 19 30 33.1 | +03 26 40 | 6.05 | A0eShell | S:He lines widened by rotation; NaI lines narrow. Also classified B9.5Ia. Line profiles vary.,VAR:Gamma Cas, amp. 0.12V, 0.8518d. Variation may be due to rotation and inhomogeneous distribution of brightness on disk. | ||||||||
HR 7429 | μ | 38 | BD+07 4132 | 184406 | 124799 | 1511 | I | 12607 | 12155 | 19 34 05.4 | +07 22 44 | 4.45 | K3-IIIbCN0.5 | 5.0 | 177.5 | D:B and C optical. | |
HR 7430 | 37 | BD-10 5122 | 184492 | 162792 | 3562 | I | 19 35 07.3 | -10 33 37 | 5.12 | G9IIIa | |||||||
HR 7432 | BD-07 4998 | 184573 | 143564 | 19 35 29.8 | -07 27 37 | 6.34 | K0 | ||||||||||
HR 7438 | BD+02 3932 | 184663 | 124823 | 19 35 25.2 | +02 54 48 | 6.38 | F6IV | ||||||||||
HR 7445 | BD+10 3981 | 184884 | 105032 | 12660 | 19 36 08.0 | +11 09 00 | 6.68 | A3V | 6.4 | 3.8 | |||||||
HR 7446 | κ | 39 | BD-07 5006 | 184915 | 143600 | 737 | I | 12204 | 19 36 53.5 | -07 01 39 | 4.95 | B0.5III | G:Sct OB2. | ||||
HR 7447 | ι | 41 | BD-01 3782 | 184930 | 143597 | 12663 | 12201 | 19 36 43.3 | -01 17 11 | 4.36 | B5III | 8.9 | 47.0 | G:Member of the local association (Pleiades group). | |||
HR 7449 | BD+14 3974 | 184944 | 105036 | 19 36 15.8 | +14 23 30 | 6.38 | K0II-III | ||||||||||
HR 7456 | BD+10 3984 | 185018 | 105045 | 12670 | 19 36 52.5 | +11 16 24 | 5.98 | G0Ib | 5.7 | 80. | |||||||
HR 7460 | 42 | BD-04 4861 | 185124 | 143621 | 19 37 47.3 | -04 38 51 | 5.46 | F3IV | |||||||||
HR 7471 | BD+03 4097 | 185423 | 124892 | 3569 | 19 38 49.0 | +03 22 54 | 6.35 | B3III | |||||||||
HR 7474 | σ | 44 | BD+05 4225 | 185507 | 124903 | 12737 | Sig Aql | 19 39 11.6 | +05 23 52 | 5.17 | B3V+B3V v | 6.6 | 47.8 | D:B, 12v K0Ve at 48" optical. C, 12v at 130". Rotational velocity of A 123k/s, of B 142k/s.,SB:ADS 12737A, 1.950271d, K 164.2k/s, V0 -4.5k/s, msin3i 5.84, asini 4.40. vsini of secondary 129k/s.,VAR:ADS 12737A, EB 5.18 - 5.36B, 1.95026827d. i 71.7d. Spectra vary in period 1.950271d. | |||
HR 7480 | 45 | BD-00 3813 | 185762 | 143678 | 3573 | 12775 | 19 40 43.3 | -00 37 16 | 5.67 | A3IV | 7.2 | 42.0 | D:A companion at 0.084" discovered by speckle interferometry. | ||||
HR 7486 | BD+13 4098 | 185936 | 105132 | 3574 | W | QS Aql | 19 41 05.5 | +13 48 56 | 6.01 | B5V | 0.2 | 0.1 | D:Speckle interferometry 1985.5 gives sep. 0.178".,G:Member of the local association (Pleiades group).,SB:2.4968d, K 47.3k/s, V0 -14.2k/s, asini 1.62. Equal components.,VAR:Primary of visual double, EA 5.93 - 6.05V, 2.513294d. Double unresolved in 1961 when period changed sharply. | ||||
HR 7493 | 46 | BD+11 3954 | 186122 | 105156 | 19 42 12.8 | +12 11 36 | 6.34 | B9IIIpHgMn | |||||||||
HR 7497 | χ | 47 | BD+11 3955 | 186203 | 105168 | 12808 | 12325 | 19 42 34.0 | +11 49 36 | 5.27 | G0:III+A3V | 1.2 | 0.4 | D:AB, fixed sep.,DYN:0.0006".,S:Also classified G2+B8 and dF3+A3. | |||
HR 7511 | ψ | 48 | BD+12 4059 | 186547 | 105199 | 19 44 34.1 | +13 18 10 | 6.26 | B9III-IV | SB:Double lines suspected. | |||||||
HR 7516 | BD-03 4701 | 186660 | 143776 | 3579 | 19 45 52.2 | -02 53 00 | 6.48 | B3III | |||||||||
HR 7519 | υ | 49 | BD+07 4210 | 186689 | 125032 | 19 45 39.9 | +07 36 48 | 5.91 | A3IV | ||||||||
HR 7525 | γ | 50 | BD+10 4043 | 186791 | 105223 | 741 | I | W | 19 46 15.6 | +10 36 48 | 2.72 | K3II e | 8.0 | 132.6 | N:TARAZED; Reda.,S:Ultraviolet FeII emission. | ||
HR 7541 | BD-11 5131 | 187195 | 163012 | 19 49 02.2 | -10 52 15 | 6.04 | K5III | ||||||||||
HR 7542 | BD+10 4058 | 187203 | 105278 | 19 48 30.4 | +10 41 39 | 6.44 | F8Ib-II | ||||||||||
HR 7544 | π | 52 | BD+11 3994 | 187259 | 105282 | 12962 | 12425 | 19 48 42.1 | +11 48 57 | 5.72 | G2III:+A1V: | 0.5 | 1.4 | D:AB, >3000y. | |||
HR 7553 | 51 | BD-11 5149 | 187532 | 163036 | 744 | 13017 | 19 50 46.8 | -10 45 49 | 5.39 | F0V | 8.0 | 21.1 | D:Optical. | ||||
HR 7554 | BD+07 4252 | 187567 | 125116 | S | V1339 Aql | 19 50 17.5 | +07 54 09 | 6.51 | B2.5IVe | 0.1 | VAR:Gamma Cas? 6.33 - 6.52V. | ||||||
HR 7557 | α | 53 | BD+08 4236 | 187642 | 125122 | 745 | I | 13009 | 19 50 47.0 | +08 52 06 | 0.77 | A7V | 8.6 | 165.2 | D:Component B optical.,N:ALTAIR; Atair.,R:Diam. = 0.00278 - 0.00298". | ||
HR 7559 | BD-02 5133 | 187660 | 143853 | I | 19 51 11.1 | -02 27 39 | 6.13 | K5III | |||||||||
HR 7560 | ο | 54 | BD+10 4073 | 187691 | 105338 | 13012 | 19 51 01.6 | +10 24 56 | 5.11 | F8V | 8.3 | 14.4 | D:Component B optical. AC, 13.8 dM4, 22" binary. | ||||
HR 7562 | BD+09 4288 | 187753 | 125139 | 19 51 17.7 | +09 37 49 | 6.25 | A1m | ||||||||||
HR 7569 | BD+11 4019 | 187923 | 105348 | W | 12490 | 19 52 03.5 | +11 37 44 | 6.13 | G0V | 5.5 | 90.5 | ||||||
HR 7570 | η | 55 | BD+00 4337 | 187929 | 125159 | 746 | I | Eta Aql | 19 52 28.4 | +01 00 20 | 3.90 | F6Ib v | S:Also classified F6Ib-G4Ib. UV suggests A0V companion.,VAR:Discovered by Pigott in 1784. CDelta 3.50 - 4.30V, 7.176641d. Period changes. Variable He 10830 in emission and,VAR:absorption. | ||||
HR 7572 | BD+09 4295 | 187961 | 105355 | 13041 | 12496 | 19 52 15.6 | +10 21 05 | 6.54 | B7V | 4.0 | 13.5 | D:Component B = A3V.,G:Member of the local association (Pleiades group). | |||||
HR 7575 | BD-03 4742 | 188041 | 143883 | 1519 | V1291 Aql | 19 53 18.7 | -03 06 52 | 5.65 | A5p v | S:Also classified F0p SrCrEu.,VAR:Alpha CV 5.61 - 5.67V, 224.5d. Also period for spectrum and magnetic field var. Rotation 226d. | |||||||
HR 7580 | BD+04 4264 | 188107 | 125182 | 19 53 22.6 | +04 24 02 | 6.53 | B9.5Vn | ||||||||||
HR 7584 | 56 | BD-08 5150 | 188154 | 143894 | I | W | 19 54 08.2 | -08 34 27 | 5.79 | gK5 | 6.1 | 46.5 | |||||
HR 7593 | 57 | BD-08 5154 | 188293 | 143898 | 13087 A | 19 54 37.6 | -08 13 38 | 5.71 | B7Vn | 0.8 | 35.7 | D:CPM with HR 7594. | |||||
HR 7594 | 57 | BD-08 5155 | 188294 | 143899 | 13087 B | 19 54 38.1 | -08 14 14 | 6.49 | B8V | 0.8 | 35.7 | D:CPM with HR 7593. | |||||
HR 7595 | ξ | 59 | BD+08 4261 | 188310 | 125210 | I | 19 54 14.9 | +08 27 41 | 4.71 | G9+IIIb | |||||||
HR 7596 | 58 | BD-00 3871 | 188350 | 125219 | 19 54 44.8 | +00 16 25 | 5.61 | A0III | |||||||||
HR 7598 | BD+06 4351 | 188385 | 125221 | 13093 | 19 54 40.3 | +07 08 25 | 6.15 | A2V | 6.4 | 13.8 | D:Optical. | ||||||
HR 7599 | BD-07 5102 | 188405 | 143911 | 13104 | 19 55 19.6 | -06 44 03 | 6.51 | F2V | 1.1 | 0.2 | D:Speckle interferometry 1985.5 gives sep. 0.173". | ||||||
HR 7602 | β | 60 | BD+06 4357 | 188512 | 125235 | 749 | I | 13110 | 12557 | 19 55 18.8 | +06 24 24 | 3.71 | G8IV | 7.7 | 175.0 | D:AB binary. B 12v dM3 at 13".,DYN:0.049".,N:ALSHAIN; Alschairn.,VAR:ADS 13110A, amp. 0.05V. | |
HR 7610 | φ | 61 | BD+11 4055 | 188728 | 105438 | 3590 | 19 56 14.3 | +11 25 26 | 5.28 | A1IV | SB:3.3207d, K 37.2k/s, V0 -28.0k/s, asini 1.70. | ||||||
HR 7636 | BD+00 4375 | 189322 | 125310 | 3596 | 19 59 22.7 | +01 22 40 | 6.17 | G8III | |||||||||
HR 7637 | BD-10 5238 | 189340 | 163168 | W | 19 59 47.4 | -09 57 30 | 5.88 | F8V | 0.0 | 0.1 | |||||||
HR 7648 | BD+08 4300 | 189695 | 125355 | I | 20 00 58.9 | +08 33 29 | 5.91 | K5III | |||||||||
HR 7661 | BD-07 5159 | 190172 | 144038 | 20 04 01.2 | -07 28 11 | 6.72 | F4III | ||||||||||
HR 7664 | BD+15 4033 | 190229 | 105615 | 20 03 30.0 | +16 01 53 | 5.67 | B9pHgMn | G:Member of the local association (Pleiades group).,N:14 Sge, in Aquila.,RV:61.7d? Earlier vsini 61k/s. | |||||||||
HR 7667 | 62 | BD-01 3887 | 190299 | 144045 | I | 20 04 23.2 | -00 42 34 | 5.68 | K4III | ||||||||
HR 7669 | τ | 63 | BD+06 4416 | 190327 | 125403 | 1524 | I | 20 04 08.3 | +07 16 41 | 5.52 | gK0 | ||||||
HR 7671 | BD-12 5641 | 190390 | 163245 | W | V1401 Aql | 20 05 05.4 | -11 35 58 | 6.34 | F1III | 25. | D:Discovered as double by W. Herschel; companion not rediscovered.,S:Probably a supergiant.,VAR:SRd 6.18 - 6.55V, 28.49d. | ||||||
HR 7680 | BD+15 4040 | 190658 | 105663 | I | 13344 | 20 05 26.5 | +15 30 01 | 6.34 | M2.5III | 4.0 | 2.7 | D:CPM. | |||||
HR 7681 | BD-04 5013 | 190664 | 144062 | 20 06 12.2 | -04 04 42 | 6.47 | K0 | ||||||||||
HR 7690 | 64 | BD-01 3899 | 191067 | 144095 | 20 08 01.8 | -00 40 42 | 5.99 | K1IV | |||||||||
HR 7693 | BD+08 4344 | 191104 | 125478 | 13403 | 20 07 50.3 | +09 23 59 | 6.43 | F3V | 2.1 | 3.1 | D:Binary. | ||||||
HR 7700 | BD+10 4189 | 191263 | 105743 | 3616 | 20 08 38.3 | +10 43 33 | 6.31 | B3V | G:Member of the local association (Pleiades group). | ||||||||
HR 7710 | θ | 65 | BD-01 3911 | 191692 | 144150 | 756 | I | W | 20 11 18.3 | -00 49 17 | 3.23 | B9.5III | 9.6 | 113.7 | G:In reflection nebula.,SB:17.1243d, K 51.0k/s, V0 -27.9k/s, msin3i 0.742, asini 9.52. | ||
HR 7717 | BD+00 4444 | 191984 | 125567 | 13506 A | 20 12 35.2 | +00 52 03 | 6.27 | B9pCrEu:Sr: | 0.2 | 2.8 | D:Discordance as to which component has the peculiar spectrum usually attributed to A. However, on the basis of better,D:spectrograms, Abt gives A = A0V, B = A0Vp(Sr,Cr st.,Ca wk.). | ||||||
HR 7720 | 66 | BD-01 3920 | 192107 | 144181 | I | 20 13 13.9 | -01 00 34 | 5.47 | K5III | S:Very bright in ultraviolet. | |||||||
HR 7724 | ρ | 67 | BD+14 4227 | 192425 | 105878 | 1526 | 20 14 16.6 | +15 11 51 | 4.95 | A2V | |||||||
HR 7768 | BD-01 3951 | 193329 | 144296 | 20 19 43.3 | -01 04 43 | 6.06 | K0 | ||||||||||
HR 7772 | BD-06 5451 | 193429 | 144313 | 3628 | I | 13013 | 20 20 26.1 | -06 21 42 | 6.63 | K5 | VAR:Amp. 0.06V. | ||||||
HR 7794 | BD+04 4434 | 194013 | 125747 | 1531 | 20 23 10.7 | +05 20 35 | 5.31 | G8III-IV | |||||||||
HR 7803 | BD+00 4495 | 194244 | 125769 | 13811 | 13064 | 20 24 37.5 | +01 04 07 | 6.15 | B9V | 4.7 | 31.3 | D:Discordances as to which component is B, which C. IDS gives B, 13.1v at 17.1". | |||||
HR 7809 | BD-03 4888 | 194454 | 144412 | 20 25 42.5 | -02 48 01 | 6.11 | gK1 | ||||||||||
HR 7821 | 68 | BD-03 4906 | 194939 | 144468 | W | 20 28 24.9 | -03 21 28 | 6.13 | B9V | 7.7 | 9.8 | ||||||
HR 7831 | 69 | BD-03 4918 | 195135 | 144495 | 1533 | I | 20 29 39.0 | -02 53 08 | 4.91 | K2III | |||||||
HR 7873 | 70 | BD-03 4961 | 196321 | 144624 | 3648 | I | 20 36 43.6 | -02 33 00 | 4.89 | K5II | |||||||
HR 7878 | BD-00 4056 | 196426 | 144632 | 20 37 18.3 | +00 05 49 | 6.22 | B8IIIp | ||||||||||
HR 7884 | 71 | BD-01 4016 | 196574 | 144649 | I | 14081 | 13187 | 20 38 20.3 | -01 06 19 | 4.32 | G7.5IIIa | 7.5 | 32.2 | D:Optical.,SB:ADS 14081A, 205.2d, K 9.8k/s, V0 -5.9k/s, asini 27.7. |
Planetary Nebulae | ||||||||
---|---|---|---|---|---|---|---|---|
Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
NGC 6741 | 19 02 37.0 | -00 26 56 | PN | 10.8 | 11.5 | 0.13 | planetary, stellar | PK 33-2.1, J 475, CS=14.7 |
NGC 6751 | 19 05 55.5 | -05 59 30 | PN | 12.5 | 11.9 | 0.43 | pB, S | NGC 6748, PK 29-5.1, CS=13.9 |
NGC 6772 | 19 14 36.4 | -02 42 22 | PN | 14.2 | 12.7 | 1.43 | vF, L, R, vvlbM, r | PK 33-6.1, CS=18.4 |
NGC 6781 | 19 18 28.3 | +06 32 25 | PN | 11.8 | 11.4 | 1.9 | planetary, F, L, R, vsbM disc, S * nf | PK 41-2.1, CS=15.0 |
NGC 6785 | 19 18 24.9 | -01 35 45 | PN | 13.3 | 12.3 | 0.62 | eS, stellar | NGC 6778, PK 34-6.1, CS=15.0 |
NGC 6790 | 19 22 57.0 | +01 30 49 | PN | 10.2 | 10.5 | 0.17 | planetary, B, eS, stell = 9.5 mag | PK 37-6.1, CS=13.5 |
NGC 6803 | 19 31 16.3 | +10 03 26 | PN | 11.3 | 11.4 | 0.17 | planetary, stellar | PK 46-4.1, CS=15.2 |
NGC 6804 | 19 31 35.4 | +09 13 33 | PN | 12.2 | 12.0 | 1.1 | cB, S, iR, rrr | PK 45-4.1, CS=14.3 |
NGC 6807 | 19 34 33.5 | +05 41 04 | PN | 13.8 | 12.0 | 0.13 | planetary, stellar | PK 42-6.1, CS=14.0 |
NGC 6852 | 20 00 39.2 | +01 43 43 | PN | 12.8 | 12.6 | 0.47 | F neb, am st | PK 42-14.1 |
IC 4846 | 19 16 28.3 | -09 02 35 | PN | 12.7 | 11.9 | 0.18 | Planetary, stellar | PK 27-9.1, CS=13.7 |
Open Clusters | ||||||||
Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
NGC 6709 | 18 51 30.0 | +10 20 00 | III2m | 6.7 | 15 | Cl, pRi, lC, iF | OCL 100 | |
NGC 6755 | 19 07 49.0 | +04 16 00 | IV2m | 7.5 | 15 | Cl, vL, vRi, pC, st 12…14 | OCL 96 | |
NGC 6756 | 19 08 42.5 | +04 42 21 | I2m | 10.6 | 4 | Cl, S, Ri, lC, st 11…12 | OCL 99 | |
NGC 6837 | 19 53 08.0 | +11 41 54 | OCL | 12.0 | 3 | Cl, S, P | OCL 108 | |
Globular Clusters | ||||||||
Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
NGC 6749 | 19 05 15.3 | +01 54 05 | GCL | 12.4 | 4 | Cl, L, lC, st L & S | GCL 107, OCL 91, Berkeley 42, not OCL (I3r) | |
NGC 6760 | 19 11 12.1 | +01 01 52 | IX | 9.0 | 9.6 | pB, pL, vglbM (Auw. 44) | GCL 109 | |
Galaxies | ||||||||
Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
NGC 6814 | 19 42 40.5 | -10 19 28 | SBbc | 12.1 | 11.2 | 3 × 2.8 | pF, pL, R, bM, r | MCG -2-50-1, IRAS 19399-1026 |
NGC 6821 | 19 44 24.2 | -06 50 04 | SBcd | 13.6 | 13.1 | 1.3 × 1.1 | F, pL, R | MCG -1-50-2, IRAS 19417-0657 |
NGC 6865 | 20 05 56.4 | -09 02 26 | S0 | 16.0 | 15.0 | 0.8 × 0.6 | F, S, E | |
NGC 6900 | 20 21 35.1 | -02 34 11 | Sb | 14.3 | 13.5 | 1 × 0.8 | vF, S, R | MCG 0-52-1, MCG -1-52-1, IRAS 20189-0243 |
NGC 6901 | 20 22 21.6 | +06 25 47 | SBab | 14.5 | 13.7 | 1.4 × 0.5 | eF | IC 5000, UGC 11542, MCG 1-52-2, CGCG 399-2, IRAS 20199+0616 |
NGC 6906 | 20 23 34.0 | +06 26 40 | SBbc | 13.2 | 12.3 | 1.6 × 0.8 | pF, pL, R | UGC 11548, MCG 1-52-3, CGCG 399-6, IRAS 20211+0616 |
NGC 6915 | 20 27 46.0 | -03 04 36 | Sab | 13.0 | 12.2 | 1.5 × 0.9 | pB, S, R | IRAS 20251-0314 |
NGC 6922 | 20 29 52.8 | -02 11 30 | Sc | 14.0 | 13.5 | 1.3 × 1 | vF, pL, R | UGC 11574, MCG 0-52-18, CGCG 373-17, IRAS 20272-0221 |
NGC 6926 | 20 33 05.9 | -02 01 44 | SBc/P | 13.2 | 12.4 | 2 × 1.4 | vF, pL, E 176°, p of 2 | UGC 11588, MCG 0-52-33, CGCG 373-33, VV 621, IRAS 20305-0211 |
NGC 6929 | 20 33 21.6 | -02 02 12 | S0-a | 14.4 | 13.4 | 0.8 × 0.7 | vF, vS, sf of 2 | MCG 0-52-35, CGCG 373-35, NPM1G -02.0441 |
NGC 6941 | 20 36 23.5 | -04 37 08 | Sb | 13.6 | 12.8 | 2 × 1.4 | eF, lE, lbM | MCG -1-52-10, IRAS 20337-0447 |
IC 1317 | 20 23 15.5 | +00 39 53 | E1 | 14.6 | 13.8 | 0.7 × 0.6 | Planetary = * 12, diam 10"-15" | UGC 11546, MCG 0-52-4, CGCG 373-5, 2ZW 82 |
IC 1327 | 20 35 41.3 | -00 00 19 | S0-a | 14.9 | 14.0 | 0.9 × 0.8 | vF, * 8 1' f | CGCG 373-38, KARA 881 |
PNG | RA | Dec | Main ID | PK | IRAS | Discoverer | Identities | oDiam ["] | rDiam ["] | Dist [kpc] | Rvel [km/s] | ExpVel [km/s] | C* Name | C* Mag | C* SP Type |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
PN G025.9-10.9 | 19 18 19 | -11 06 12 | Na 2 | 26-11.1 | 19155-1111 | NASSAU 1964 | AS 350, MHa 319- 34, Sa 2-387 | 16. : | AG82 360, AS 350 | WR | |||||
PN G027.6-09.6 | 19 16 28 | -9 02 37 | IC 4846 | 27-09.1 | 19137-0908 | FLEMING 1901 | ARO 103, AS 348, VV 226, VV' 488, Sa 2-385 | 2. | 2.9 | +151.0 ± 3.0 | 13.1 (O-III) | AG82 357, AS 348, BD -09 5069, GCRV 11715, HD 180324 | B: 15.19, V: 15.19 | Of | |
PN G029.2-00.0 | 18 44 53 | -3 20 34 | TDC 1 | THOMPSON et al 1991 | IR 29.211 | 5.6 | 6. | -55. ± 60. | |||||||
PN G029.2-05.9 | 19 05 56 | -5 59 28 | NGC 6751 | 29-05.1 | 19032-0604 | FLEMING 1907 | ARO 101, Sa 2-382, Th 1- J, VV 219, VV' 477 | 20.5 | 1.4 | -38.5 ± 2.8 | 40.0 (O-III), 38. (N-II) | AG82 344, CSI -06 -19031 0, EM* CDS 1043, HD 177656 | B: 15.78, V: 15.45 | WC 4 | |
PN G029.8-07.8 | 19 13 56 | -6 18 51 | LSA 1 | LUNDSTROM et a 1988 | 14. | ||||||||||
PN G031.0-10.8 | 19 27 02 | -6 34 54 | M 3-34 | 31-10.1 | 19243-0641 | MINKOWSKI 1948 | ARO 322, Sa 2-390, VV' 498 | 5.6 | 8. | +37.0 ± 25.0 | 14.0 (O-III) | AG82 369 | B: 16.2, V: 16.3 | ||
PN G031.3-00.5 | 18 50 25 | -1 40 09 | HaTr 10 | HARTL et al 1983 | S 2-68 | 25. | |||||||||
PN G031.9-00.3 | 18 50 40 | -1 03 14 | WeSb 4 | WEINBERGER et al 1981 | 30. | ||||||||||
PN G032.0-03.0 | 19 00 34 | -2 11 57 | K 3-18 | 32-03.1 | 18579-0216 | KOHOUTEK 1964 | ARO 299, Sa 3-152 | 4. | 0.9 | ||||||
PN G032.5-03.2 | 19 02 10 | -1 48 40 | K 3-20 | 32-03.2 | 18595-0153 | KOHOUTEK 1964 | Sa 3-153 | 0. | V: 17.0 | ||||||
PN G032.7-02.0 | 18 58 26 | -1 03 46 | M 1-66 | 32-02.1 | 18558-0107 | MINKOWSKI 1946 | Sa 2-378, VV 216, VV' 470 | < 10. | 2.7 | +42.6 ± 10.1 | |||||
PN G032.9-02.8 | 19 01 37 | -1 19 08 | K 3-19 | 32-02.2 | 18590-0123 | KOHOUTEK 1964 | ARO 301, Sa 2-379 | 0. | 1.2 | ||||||
PN G033.0-05.3 | 19 10 30 | -2 21 02 | A 55 | 33-05.1 | 19078-0225 | ABELL 1955 | A55 43, VV' 480 | 62. | 48. | AG82 347 | B: 20.5 | ||||
PN G033.1-06.3 | 19 14 28 | -2 42 26 | NGC 6772 | 33-06.1 | 19119-0247 | PICKERING 1879 | ARO 102, Sa 2-384, VV 224, VV' 486 | 64. | 90. | 1.3 : | 0.0 ± 4.0 | 10.2 (O-III), 25. (N-II) | AG82 355 | B: 19.02, V: 18.68 | |
PN G033.2-01.9 | 18 58 50 | +0 41 15 | Sa 3-151 | 18563-0037 | SANDULEAK 1976 | 0. | B: 14.89, V: 14.00 | A | |||||||
PN G033.8-02.6 | 19 02 35 | +0 35 37 | NGC 6741 | 33-02.1 | 19000-0031 | PICKERING 1885 | ARO 53, J 475, Sa 2-380, VV 217, VV' 474 | 8. | 6. | 2.1 | +41.3 ± 1.4 | 23.0 (O-III), 21.5 (N-II) | AG82 340 | B: >20.3 | |
PN G034.0+02.2 | 18 45 24 | +2 01 23 | K 3-13 | 34+02.1 | 18428+0158 | KOHOUTEK 1964 | ARO 290 | 0. | 3.7 | ||||||
PN G034.1-10.5 | 19 31 07 | -3 42 24 | HDW 11 | HARTL et al 1983 | HaWe 13 | 47. | AG82 371 | B: 16.6 | |||||||
PN G034.5-06.7 | 19 18 25 | -1 35 53 | NGC 6778 | 34-06.1 | 19158-0141 | PICKERING 1882 | ARO 72, Sa 2-388, VV 227, VV' 491 | 15.8 | 1.0 | +91.0 ± 3.0 | 20.0 (O-III) | AG82 362, CSI -01 -19156, HD 180871, PLX 4502 | B: 16.91 | ||
PN G035.1-00.7 | 18 58 08 | +1 37 06 | Ap 2-1 | 35-00.1 | APRIAMASVILI 1962 | ARO 143 | 32.8 | B: 16.96, V: 15.16 | |||||||
PN G035.7-05.0 | 19 14 40 | +0 13 37 | K 3-26 | 35-05.1 | 19120+0008 | KOHOUTEK 1964 | ARO 309 | 10. | |||||||
PN G035.9-01.1 | 19 01 00 | +2 09 23 | Sh 2- 71 | 36-01.1 | 18594+0204 | SHARPLESS 1959 | ARO 31, V-V 1-9, VV'473 | 100. | 114. | +24.7 ± 3.0 | 16.0 (O-III), 21.5 (N-II) | AG82 339 | U: 14.97, B: 14.59, V: 13.75 | B | |
PN G036.9-01.1 | 19 02 59 | +3 02 21 | HaTr 11 | HARTL et al 1983 | 12. | ||||||||||
PN G036.9-02.6 | 19 08 02 | +2 21 24 | HaTr 13 | HARTL et al 1983 | 21. | ||||||||||
PN G037.5-05.1 | 19 18 20 | +1 46 51 | A 58 | 37-05.1 | 19158+0141 | ABELL 1955 | A55 45, ARO 150, VV' 489 | 40. | AG82 361, AN 7.1920, C* 2719, NOVA AQL 1919, V605 Aql | WC early | |||||
PN G037.8-06.3 | 19 22 57 | +1 30 47 | NGC 6790 | 37-06.1 | PICKERING 1882 | ARO 33, VV 229, VV' 496 | 7. | 1.8 | 1.3 | +40.4 ± 1.7 | 15.0 (O-III) | AG82 366, BD +01 3979, GCRV 11824, HD 182083, NSV 11959, SON 9934 | B: 11.1 | WN? | |
PN G037.9-03.4 | 19 13 07 | +2 52 49 | A 56 | 37-03.2 | ABELL 1955 | A55 44, ARO 146, VV' 483 | 181. | AG82 352 | B: 19.7 | ||||||
PN G038.1-25.4 | 20 31 33 | -7 05 21 | A 70 | 38-25.1 | ABELL 1955 | A55 57, ARO 351, VV' 536 | 42. | -79.0 ± 18.0 | 37.8 (O-III) | AG82 410 | B: 19.1 | ||||
PN G038.4-03.3 | 19 13 23 | +3 25 03 | K 4-19 | 38-03.1 | 19108+0319 | KOHOUTEK 1964 | 0. | B: 15.55, V: 14.72 | |||||||
PN G038.7-03.3 | 19 13 54 | +3 37 45 | M 1-69 | 38-03.2 | 19113+0332 | MINKOWSKI 1946 | ARO 187, VV 223, VV' 485 | 0. | +7.0 ± 25.0 | 25.0 (O-III), 30.0 (N-II) | |||||
PN G039.5-02.7 | 19 13 34 | +4 38 06 | M 2-47 | 39-02.1 | 19110+0432 | MINKOWSKI 1947 | ARO 147, VV 222, VV' 484 | 6.4 | 6. | +36.0 ± 11.4 | 11.5 (O-III) | AG82 353 | B: 18.3, V: 17.3 | ||
PN G039.8+02.1 | 18 56 18 | +7 07 23 | K 3-17 | 39+02.1 | 18538+0703 | KOHOUTEK 1964 | ARO 297 | 14.8 | 8. | ||||||
PN G040.3-00.4 | 19 06 46 | +6 23 56 | A 53 | 40-00.1 | 19043+0619 | ABELL 1955 | A55 41, ARO 183, VV' 478 | 31. | AG82 345 | B: 20.9 | |||||
PN G040.4-03.1 | 19 16 28 | +5 13 19 | K 3-30 | 40-03.1 | 19140+0507 | KOHOUTEK 1964 | ARO 312 | 0. | 3.3 | ||||||
PN G041.2-00.6 | 19 09 13 | +7 05 43 | HaTr 14 | HARTL et al 1983 | 18. | ||||||||||
PN G041.8+04.4 | 18 51 41 | +9 54 52 | K 3-15 | 41+04.1 | 18493+0951 | KOHOUTEK 1964 | ARO 294 | 0. | < 0.3 | ||||||
PN G041.8-02.9 | 19 18 28 | +6 32 23 | NGC 6781 | 41-02.1 | 19160+0626 | HERSCHEL 1830 | ARO 32, VV 228, VV' 492 | 108. | 130. | 1.6 | +4.3 ± 3.7 | 12.0 (O-III) | AG82 363 | B: 17.10, V: 16.78 | |
PN G042.0+05.4 | 18 48 33 | +10 35 51 | K 3-14 | 42+05.1 | 18461+1032 | KOHOUTEK 1964 | AS 324, MHa 352- 9 | 0. | 1. | V: 16.2 | |||||
PN G042.5-14.5 | 20 00 40 | +1 43 52 | NGC 6852 | 42-14.1 | 19581+0135 | KOHOUTEK 1963 | ARO 167, K 1-18 | 28. | -11.0 ± 5.0 | 43.1 (O-III) | B: 17.70, V: 17.90 | ||||
PN G042.9-06.9 | 19 34 33 | +5 41 02 | NGC 6807 | 42-06.1 | 19320+0534 | PICKERING 1882 | ARO 74, VV 234, VV' 502 | 2. | 0.8 | -67.7 ± 3.3 | 13.0 (O-III) | AG82 375, BD +05 4196, LF 1 +05 175 | B: 16.3 | ||
PN G043.0-03.0 | 19 21 01 | +7 36 59 | M 4-14 | 43-03.1 | MINKOWSKI 1948 | ARO 120 | 7.4 | 7. | +48.0 ± 11.0 | ||||||
PN G043.1+03.8 | 18 56 33 | +10 52 14 | M 1-65 | 43+03.1 | 18541+1048 | MONKOWSKI 1946 | ARO 142, VV 215, VV' 467 | 3.6 | 4.0 | +20.0 ± 11.0 | 11.5 (N-II) | AG82 336 | B: 15.30, V: 14.89 | ||
PN G043.3+02.2 | 19 02 18 | +10 17 24 | PM 1-276 | PREITE-MARTINEZ 1988 | CTSS 1 | 14. | B: 19.5, V: 18.5 | ||||||||
PN G043.5-13.4 | 19 58 29 | +3 02 23 | A 67 | 43-13.1 | ABELL 1955 | A55 54, ARO 117, VV' 520 | 67. | AG82 390 | B: 19.3 | ||||||
PN G044.3-05.6 | 19 32 39 | +7 27 58 | K 3-36 | 44-05.1 | 19302+0721 | KOHOUTEK 1964 | 12. | B: 17.2, V: 17.3 | |||||||
PN G045.4-02.7 | 19 24 22 | +9 53 55 | Vy 2- 2 | 45-02.1 | 19219+0947 | VYSSOTSKY 1945 | ARO 151, M 1-70, VV 230, VV' 497 | 14. | 0.5 | -71.4 ± 3.9 | 17.5 (O-III), 25.0 (N-II) | AG82 367 | B: 15.51, V: 14.60 | ||
PN G045.6+01.5 | 19 09 26 | +12 00 48 | K 3-22 | 45+01.1 | KOHOUTEK 1964 | 0. | |||||||||
PN G045.7-04.5 | 19 31 36 | +9 13 38 | NGC 6804 | 45-04.1 | 19291+0907 | PEASE 1917 | ARO 34, VV 233, VV' 500 | 35. | 1.1 | -12.0 ± 3.8 | 24.0 (O-III) | AG82 373, CSI +09 -19291, HD 183932, PLX 4568 | B: 14.47, V: 14.37 | O9, O(H) | |
PN G045.9-01.9 | 19 22 27 | +10 41 21 | K 3-33 | 45-01.1 | 19200+1035 | KOHOUTEK 1964 | 0. | 1.1 | |||||||
PN G046.3-03.1 | 19 27 45 | +10 24 21 | PB 9 | 46-03.1 | 19253+1018 | PEIMBERT et al 1960 | ARO 152 | 12. : | 9.0 | ||||||
PN G046.4-04.1 | 19 31 16 | +10 03 24 | NGC 6803 | 46-04.1 | 19289+0956 | PICKERING 1882 | ARO 73, VV 232, VV' 499 | 5.5 | 2.4 | 3.0 | +13.1 ± 1.8 | 14.5 (O-III), 20. (N-II) | AG82 372, CSI +09 -19289, EM* CDS 1073, HD 183889 | V: 15.2 | WN? |
PN G046.8+02.9 | 19 06 23 | +13 44 41 | CTSS 4 | CAPELLARO et al 1990 | 10. | ||||||||||
PN G046.8+03.8 | 19 03 08 | +14 06 58 | CTSS 3 | CAPELLARO et al 1990 | Sh 2-78 | 600. | B: 17.98, V: 17.78 | ||||||||
PN G047.1+04.1 | 19 02 40 | +14 28 52 | K 3-21 | 47+04.1 | KOHOUTEK 1964 | 7.2 | B: 18.6, V: 16.9 | ||||||||
PN G047.1-04.2 | 19 33 18 | +10 37 01 | A 62 | 47-04.1 | ABELL 1955 | A55 50, ARO 155, VV' 501 | 161. | 13. (O-III), 24. (N-II) | AG82 374 | B: 18.8 | |||||
PN G048.0-02.3 | 19 28 14 | +12 19 37 | PB 10 | 48-02.1 | 19258+1213 | PEIMBERT et al 1960 | Ap 4- 1, ARO 153 | 10. | 8.0 | ||||||
PN G048.1+01.1 | 19 15 30 | +14 03 50 | K 3-29 | 48+01.2 | 19132+1358 | KOHOUTEK 1964 | 0. | 1. | |||||||
PN G048.5+04.2 | 19 04 51 | +15 47 36 | K 4-16 | 48+04.2 | 19025+1542 | KOHOUTEK 1964 | ARO 303 | 0. | 3. | ||||||
PN G048.7+01.9 | 19 13 38 | +14 59 30 | He 2-429 | 48+01.1 | 19113+1454 | HENIZE 1964 | ARO 148, M 4-13 | 4.2 | +14.0 ± 11.0 | WC | |||||
PN G048.7+02.3 | 19 12 06 | +15 09 01 | K 3-24 | 48+02.1 | 19098+1504 | KOHOUTEK 1964 | ARO 305 | 6.2 | |||||||
PN G048.7-01.5 | 19 26 26 | +13 19 42 | DeHt 4 | DENGEL et al 1980 | 40. | AG82 368 | |||||||||
PN G049.4+02.4 | 19 13 05 | +15 46 42 | He 2-428 | 49+02.1 | 19108+1541 | HENIZE 1964 | ARO 186, M 4-12 | 9.6 | 8. | ||||||
PN G050.4+05.2 | 19 04 32 | +17 57 10 | A 52 | 50+05.1 | 19023+1752 | ABELL 1955 | A55 40, ARO 144, VV' 476 | 37. | AG82 342 | B: 18.4 | |||||
PN G050.4-01.6 | 19 30 17 | +14 47 22 | K 4-28 | 50-01.1 | 19279+1441 | KOHOUTEK 1964 | 0. | 0.6 | |||||||
PN G051.0-04.5 | 19 42 03 | +13 50 39 | PC 22 | 51-04.1 | 19397+1343 | APRIAMASVILI 1959 | ARO 160, VV' 508 | 20. : | B: 18.8, V: 18.1 | ||||||
PN G051.9-03.8 | 19 41 09 | +14 56 54 | M 1-73 | 51-03.1 | 19388+1449 | MINKOWSKI 1946 | ARO 158, He 2- 443, VV 238, VV' 506 | 5. | 6. | +6.9 ± 10.1 | 11.0 (O-III) | B: 15.01, V: 14.54 | |||
PN G052.2-04.0 | 19 42 19 | +15 09 05 | M 1-74 | 52-04.1 | 19400+1502 | MINKOWSKI 1946 | ARO 162, He 2- 445, VV 240, VV' 510 | < 5. | 1.0 | +10.0 ± 25.0 | 12.5 (O-III), 22.0 (N-II) | AG82 380 | B: 18.5, V: 18.1 | WN b? | |
PN G052.5-02.9 | 19 39 10 | +15 56 50 | Me 1-1 | 52-02.2 | 19368+1549 | MERRILL 1942 | ARO 104, He 2- 441, VV' 505, VV 237 | < 8. | 4.7 | -6.0 ± 7.0 | 9.0 (O-III) | B: 15.57, V: 14.12 | |||
PN G052.9-02.7 | 19 39 18 | +16 21 17 | K 3-41 | 52-02.1 | 19370+1613 | KOHOUTEK 1964 | ARO 328 | 0. | 0.5 | ||||||
PN G054.1-12.1 | 20 15 09 | +12 42 07 | NGC 6891 | 54-12.1 | 20127+1233 | COPELAND 1884 | ARO 37, VV 253, VV' 529 | 15. | 0.83 | +42.4 ± 1.0 | 7.0 (O-III) | AG82 403, BD +12 4266, EM* CDS 1140, GCRV 12622, HD 192563 | B: 12.30, V: 12.42 | Of (H) |
ID | Name | RA | Dec | RSun [kpc] | RGC [kpc] | Fe/H | wt | EB-V | VHB | (m-M)V | Vt | MV,t | U-B | B-V | V-R | V-I | spt | ellip | vr [km/s] | vLSR [km/s] | sigv [km/s] | c | rc ['] | rh ['] | μV | ρ0 | lg(tc) | lg(th) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
GLIMPSE01 | 18 48 49.7 | -01 29 50 | 4.2 | 4.9 | 0 | 4.85 | 28.80 | 28.15 | 22.24 | -5.91 | 1.37 | 0.59 | 0.65 | 7.89 | ||||||||||||||
NGC 6749 | 19 05 15.3 | +01 54 03 | 7.9 | 5.0 | -1.60 | 1 | 1.50 | 19.70 | 19.14 | 12.44 | -6.70 | 0.80 | 2.14 | -61.7 ± 2.9 | -47.2 | 0.79 | 0.62 | 1.10 | 21.88 | 3.30 | 8.59 | 8.78 | ||||||
NGC 6760 | 19 11 12.01 | +01 01 49.7 | 7.4 | 4.8 | -0.40 | 3 | 0.77 | 17.46 | 16.72 | 8.88 | -7.84 | 1.09 | 1.66 | 1.01 | 2.12 | G5 | 0.04 | -27.5 ± 6.3 | -13.2 | 1.65 | 0.34 | 1.27 | 18.66 | 3.89 | 7.96 | 9.01 | ||
Pal 11 | 19 45 14.4 | -08 00 26 | 13.4 | 8.2 | -0.40 | 4 | 0.35 | 17.46 | 16.72 | 9.80 | -6.92 | 1.27 | -68.0 ± 10.0 | -56.0 | 0.57 | 1.19 | 1.46 | 19.72 | 2.29 | 9.61 | 9.34 |