Constellation Auriga (Charioteer)

Properties
Auriga is a striking constellation north of Taurus and Gemini and is roughly the shape of a pentagon. This formation shares a star with Taurus: γ Aurigae is also the northern horn of the bull and is recorded as β Tauri, El Nath (the horn). In most atlases one finds this star belonging to Taurus. A few degrees southwest of Capella is a small, pointed triangle, the tip of which points to the north. This formation is known as The Goatling which the Charioteer carries in his arms and is formed by ε, η, and θ Aurigae. [85]
The star Capella forms together with Aldebaran (α Tauri), Rigel (β Orionis), Sirius (α Canis Maior), Procyon (α Canis Minoris) and the two twin stars Castor and Pollux (α and β Geminorum) the winter hexagon. The area of the constellation Auriga is 657 square degrees and the center culminates around midnight on December 9th. [9, 15]
Stars with Proper Names:
- α Aur: Capella, Alhajoth
- β Aur: Menkalinan, Menkalina
- ε Aur: Al Anz, Almaaz
- ζ Aur: Haedi, Haedus, Hoedus I
- η Aur: Hoedus II
- ι Aur: Hassaleh
Deep-Sky Object Descriptions
Mythology and History
The constellation has been known as the Charioteer since Babylonian times. Two different images are superimposed, reminiscent of two different incidents: It depicts a carter carrying a goat with young billy goats on his shoulders.
The goat is reminiscent of Zeus' earliest youth: At the beginning of the earliest existence, when there was still chaos, an empty space, the origin of all things, the broad-chested earth emerged. She gave birth to Uranus, heaven, so that it would surround her and so that the gods might find a permanent home there one day. She even united with Uranus herself and gave birth to the Titans. Uranos wasn't exactly a loving father, because he hated his children, cast them into the gorges of the earth and was still happy about them. One of the titans, Kronos, who was also called the crooked-minded man, horrified himself on his father with a toothed sickle sword. Uranus lost his manhood and Kronos gained dominion in heaven. Such a deed could not go unpunished and so it was made known to him through a prophecy that his own son would conquer him and deprive him of rule. Kronos, worried about his future, killed and devoured all of his newborn sons.
The nymph Amaltheia, who lived in springs and waters, was well known on the Cretan Ida. She was able to secretly take one of the children away and hid it from his cruel father in the woods. She baptized the child in the name of Zeus. Amaltheia owned a beautiful goat, the mother of two goats. This goat stood out among the dictaean herds because it had high horns bent towards its back and an udder like the one Zeus' nurse had to have. She gave her milk to God; but then she broke off a horn on a tree and was deprived of half of its ornament. The nymph took the horn, wreathed it with fresh green, filled it with fruit and raised it to Zeus' face. When he was in control of heaven, sitting on his father's throne and nothing was stronger than the undefeated Zeus, he turned his wet nurse and the cornucopia, which still bears the name of his mistress, into stars. The brightly shining capella is this goat star and underneath there are two slightly smaller stars in which you can see the goats. [20]
The charioteer was not a coachman, but rather a leader of a racing car or perhaps a chariot who drove a team of four. Some say it meant Phaethon, who borrowed the sun chariot from his father, the sun god, and in his youthful arrogance almost set the whole earth and also the sky on fire. The traces of fire can still be seen today as a band of the Milky Way and you can see how far the sun car had strayed from its path back then. [20]

In addition to Phaethon, one also believes to see another charioteer in the carter, namely Erichthonius, the son of Hephaestus who was conceived without a mother. Hephaestus was the god of fire and the artful craftsmanship, was the limping son of Zeus and Hera. Athena once came to him, the virgin goddess of war, science and the arts. Hephaestus fell in love with her and tried to rape Athena, who was fighting with all his might. His seed flowed on the earth and the virgin Athena stepped on it with shameful anger. So the goddess of the earth received him and finally gave birth to the boy Erichthonius, whom she later handed over to Athena. This boy had snake feet. Athena raised the child by keeping it in a chest guarded by snakes. He grew up to be a man and became king. Erichthonius invented a chariot because he was ashamed to show his feet. The chariot was almost similar to the sun chariot, and Zeus was so impressed by this invention that he took Erichthonius to the sky as a furman and charioteer. [20, 85]
The Roman astronomical poet Hyginus saw another person in this star of the carter: Myrtilus or Myrtilos. The king of Oinomaos of Pisa had three sons and a daughter named Hippodameia with his wife Sterope. He owned a famous stud farm and was an invincible driver of horse racing cars. King Oinomaos was warned by an oracle that his son-in-law would kill him and so he tried to prevent Hippodameia's marriage. Every young man who tried to get Hippodameia had to go through a chariot race with their father. However, should he be overtaken by the king, he would have to die by the king's spear; so it was agreed. Twelve princes had already been killed and their severed heads adorned the palace gates. Pelops, the son of the Lydian king Tantalus, also wanted to free Hippodameia and asked Poseiden, the Greek god of the seas, the fastest chariot in the world, which could also race over sea waves. Arrived in front of the palace gate and given the gruesome framing of the driveway, his courage failed. So he made use of a ruse: he promised Myrtilus - that was the king's charioteer, who was himself in love with the beautiful Hippodameia - half of his future kingdom and the right to sleep with Hippodameia on their wedding night, if he could in some way Successfully hamper the king's racing car. Myrtilos, inspired by sweet thoughts, secretly removed the pins from the axles of the wheels and replaced them with wax replicas. What happened next is easy to imagine: The king's racing car lost its wheels at full speed and the king was killed in the process. When Myrtilos wanted to claim his right to the wedding night, Pelops pushed him into the sea, where he drowned. Hermes, he was the father of Myrtilus, could not prevent this crime in time; he therefore placed him among the stars as the constellation of the charioteer. [20]
The original Greek name of this constellation was Heniochus (The One Who Holds the Reins). Other names for this constellation were Phaethon, Bellerophon, but also Custos caprarum, i.e. the goat keeper. What is meant is the goat that Zeus once served as a wet nurse. [20]
Catalogs
HR | B | F | DM | HD | SAO | FK5 | IR | M* | ADS | VarID | RA | Dec | vMag | spType | dMag | Sep ["] | Remarks |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
HR 1501 | BD+32 827 | 29867 | 57393 | 04 43 48.3 | +32 51 55 | 6.45 R | A8V | ||||||||||
HR 1528 | BD+32 840 | 30453 | 57444 | S | 04 49 19.0 | +32 35 18 | 5.86 | A8m | SB:7.0507d, K 57.8k/s, V0 +20.3k/s, asini 5.60. | ||||||||
HR 1529 | BD+31 816 | 30454 | 57441 | 2359 | I | 04 49 12.8 | +31 26 14 | 5.58 | K2III | ||||||||
HR 1535 | BD+48 1162 | 30557 | 39799 | 2361 | 04 51 09.3 | +48 44 27 | 5.66 | G9III | |||||||||
HR 1550 | BD+42 1081 | 30823 | 39826 | 04 52 47.8 | +42 35 12 | 5.71 | A3III | ||||||||||
HR 1551 | 2 | BD+36 952 | 30834 | 57475 | I | 04 52 38.0 | +36 42 11 | 4.78 | K2.5IIIbBa0.4 | G:Sirius group; UMa stream. | |||||||
HR 1558 | BD+43 1116 | 31069 | 39851 | 04 54 51.3 | +44 03 39 | 6.08 | A0V | ||||||||||
HR 1573 | BD+35 930 | 31327 | 57511 | 04 56 19.9 | +36 10 08 | 6.07 | B2Ib | G:Aur OB1. | |||||||||
HR 1577 | ι | 3 | BD+32 855 | 31398 | 57522 | 181 | I | 1778 | 04 56 59.6 | +33 09 58 | 2.69 | K3II | N:Hassaleh in Becvar.,VAR:4.0 - 4.15p. | ||||
HR 1592 | ω | 4 | BD+37 1005 | 31647 | 57548 | 3572 | 04 59 15.4 | +37 53 25 | 4.94 | A1V | 2.8 | 5.1 | D:Binary.,DYN:0.021".,G:Pleiades group. | ||||
HR 1599 | 5 | BD+39 1133 | 31761 | 57559 | 3589 | 05 00 18.3 | +39 23 41 | 5.95 | F5V | 3.4 | 3.7 | DYN:0.037". | |||||
HR 1602 | 6 | BD+39 1134 | 31780 | 57560 | I | 05 00 23.2 | +39 39 18 | 6.58 R | K4I | ||||||||
HR 1605 | ε | 7 | BD+43 1166 | 31964 | 39955 | 183 | I | 3605 | Eps Aur | 05 01 58.1 | +43 49 24 | 2.99 | F0Iae+B v | 6.2 | 207.6 | D:ADS 3605A. A* 2.98 var. A8Iap. Five visual and one astrometric components. AB visual binary, B, 14v at 29"; C,,D:11.26V, +1.83(B-V), +1.31(U-B), at 43"; D, 12.0v at 46".,N:Al Anz; Almaaz.,S:Shell star. Also classified A8Ia-F2epIa + B.,SB:ADS 3605A, 9890d, K 15.0k/s, V0 -1.4k/s, msin3i 16.8, asini 2000. Unresolved by speckle interferometry.,VAR:ADS 3605A, EA 2.94 - 3.83V, 9892d. Spectrum var. even outside eclipse. RV and light fluctuations about 110d. | |
HR 1612 | ζ | 8 | BD+40 1142 | 32068 | 39966 | 1137 | I | Zet Aur | 05 02 28.7 | +41 04 33 | 3.75 | K4II+B8V | N:Haedi; Haedus; Hoedus I. With HR 1641, one of the "kids"; Sadatoni; Saclateni.,S:Also classified K5II + B5V.,SB:972.162d, K 24.6k/s, V0 +12.9k/s, msin3i 7.54, asini 300. Unresolved by speckle interferometry . SKYLAB,SB:indicates cool star with hot companion.,VAR:EA 3.70 - 3.97V, 972.164d, i 90d. Variable duration of min. Amp. depends on wavelength, 0.55B, 1.97U. K component,VAR:amp. 0.05V. | ||||
HR 1615 | BD+41 1044 | 32188 | 39979 | 1810 | 05 03 18.6 | +41 26 30 | 6.14 | A2IIIShell? | S:H alpha, beta and gamma have absorption cores. TiII and FeII stronger than normal; MgII, SiII strong. Shell doubtful. | ||||||||
HR 1626 | BD+30 772 | 32406 | 57610 | 05 04 14.5 | +30 29 41 | 6.14 | K0II-III | ||||||||||
HR 1627 | BD+32 879 | 32428 | 57614 | 05 04 36.9 | +32 19 13 | 6.62 | A4m | S:Also classified A8.5Vm: | |||||||||
HR 1637 | 9 | BD+51 1024 | 32537 | 25019 | 3675 | 05 06 40.6 | +51 35 52 | 5.00 | F0V | 4.4 | 90.1 | D:A,B,C, CPM; D, optical; E, 12.3v at 132" from A.,SB:ADS 3675A, 391.7d, K 5.8k/s, V0 -7.4k/s, asini 29.0. | |||||
HR 1639 | BD+35 973 | 32608 | 57629 | 2379 | 05 06 00.9 | +35 56 11 | 6.52 | A5V | |||||||||
HR 1641 | η | 10 | BD+41 1058 | 32630 | 40026 | 185 | 1822 | 05 06 30.9 | +41 14 04 | 3.17 | B3V | G:Cas-Tau OB1; member of Pleiades group.,N:Hoedus II. One of the kids, with HR 1612.,RV:Doubtful var., 24d period not confirmed.,VAR:Beta C? | |||||
HR 1644 | BD+42 1170 | 32655 | 40029 | 05 06 49.6 | +43 10 29 | 6.20 | F2IIp: | ||||||||||
HR 1668 | BD+46 970 | 33167 | 40077 | 05 10 42.9 | +46 57 44 | 5.68 | F5V | G:Hyades moving group. | |||||||||
HR 1669 | BD+37 1067 | 33203 | 57704 | I | 3734 | 05 10 18.9 | +37 18 07 | 6.02 | K3:+B2II: | 0.1 | 1.5 | D:AB, CPM. | |||||
HR 1689 | μ | 11 | BD+38 1063 | 33641 | 57755 | 192 | 05 13 25.7 | +38 29 04 | 4.86 | A4Vm | |||||||
HR 1692 | BD+53 872 | 33654 | 25087 | 2393 | 05 14 44.3 | +53 12 50 | 6.20 | A0V | |||||||||
HR 1706 | 14 | BD+32 922 | 33959 | 57799 | 3824 A | KW Aur | 05 15 24.4 | +32 41 16 | 5.02 | A9IVDel Del | 2.9 | 14.3 | D:AC binary. B, 11v F4V at 13" optical.,G:Possible new Eggen group with HR 63, q.v.,SB:ADS 3824A, 3.788506d, K 23.0k/s, V0 -9.8k/s, asini 1.20.,VAR:Delta Sct 4.94 - 5.10V, 0.088088d. Form of light curve varies. Also nonradial pulsations of 0.096533 and 0.088243d. | ||||
HR 1707 | BD+53 882 | 34019 | 25112 | I | 3845 | R Aur | 05 17 17.8 | +53 35 10 | 6.50 | M7IIIe | 2.1 | 46.4 | D:Binary. Component B, 9.50V, +0.47(B-V), +0.09(U-B), F4IV.,S:Probable SiO maser emission.,VAR:ADS 3845A, M 6.7 - 13.7v, 457.64d, period changes; 10.18 - 13.12V, -0.06 to -0.43(U-B). Cycle of 64.5d also possible. | ||||
HR 1708 | α | 13 | BD+45 1077 | 34029 | 40186 | 193 | I | 3841 | 1897 | 05 16 41.4 | +45 59 53 | 0.08 | G5IIIe+G0III v | 0.5 | 0.0 | D:AP 0.6 G5III, 1.1 G0III, sep. 0.04", 0.285y, a = 0.054", masses 2.67 and 2.55 solar. Combined mag., colors. Capella is,D:first star for which an orbit was determined from interferometer measures, by Anderson at Mt. Wilson in 1920. Speckle,D:sep. 0.040" 1981.24 and 1981.68; 0.055" 1982.16. CPM with component H, a close binary, 10.0 dM1, 13.7 dM5 sep. 2" at,D:723" from A, probably physical with A. Other components all faint and distant from A.,DYN:0.058".,G:Hyades group.,N:CAPELLA; Alhajoth.,R:Diam. component A = 0.0052", component B = 0.0040".,S:Chromospheric He 10830 double. Balloon-borne spectrometer revealed pronounced emission of MgII. Soft X-ray emission.,S:Lithium content of the F-type component is 15 times that of the G component. Also classified G6III+F9III.,SB:104.0204d, K 26.1k/s, V0 +29.5k/s, asini 37.3.,VAR:Amp. 0.03V. Variable helium and X-ray emission. | |
HR 1712 | BD+34 980 | 34078 | 57816 | 3843 | AE Aur | 05 16 18.2 | +34 18 43 | 5.96 | O9.5V e | 3.3 | 8.4 | D:Component B doubtful, possibly the nebula. C 10.7V at 30".,G:Runaway star from Ori OB1 association. Moving at 128k/s in opposite direction from Mu Col = HR 1996. See HR 938.,G:Exciting star of HII region S229; associated with nebula IC 405. S229 superimposed on S230. In reflection nebula. The,G:best example of nebulosity in which the gas and dust are differently distributed.,S:Central Balmer emission in blue-violet only.,VAR:ADS 3843A, Ina 5.78 - 6.08V. Possibly a SN 2.5 million yrs. ago. | |||||
HR 1722 | BD+42 1239 | 34269 | 40214 | I | PU Aur | 05 18 15.9 | +42 47 32 | 5.48 | M4III | VAR:Lb?, amp. 0.10V. | |||||||
HR 1725 | BD+40 1240 | 34332 | 40224 | 05 18 40.4 | +40 27 54 | 6.18 | K0 | ||||||||||
HR 1726 | 16 | BD+33 1000 | 34334 | 57853 | I | 3872 | 1909 | 05 18 10.7 | +33 22 18 | 4.54 | K2.5IIIbFe-1 | 5.8 | 4.2 | D:CPM.,S:Also classified K2.5IIIb CN-0.5.,SB:ADS 3872A, 434.8d, K 14.8k/s, V0 -27.5k/s, asini 88.0.,VAR:ADS 3872A, E? | |||
HR 1728 | 17 | BD+33 1002 | 34364 | 57858 | AR Aur | 05 18 18.9 | +33 46 02 | 6.14 | B9.5V | D:Possible CPM with HR 1732.,G:Aur OB1. Concentration of hydrogen emission in direction of this association.,S:Also classified ApHgMn + B9V.,SB:4.1346d, K 107.2k/s, V0 +25.1k/s, msin3i 2.48, asini 6.09; vsini of secondary 62k/s.,VAR:EA 6.15 - 6.82V, 6.05 - 6.72B, A0 + A0, 4.134695d, changing period. | |||||||
HR 1729 | λ | 15 | BD+39 1248 | 34411 | 40233 | 1145 | 3886 | 05 19 08.5 | +40 05 57 | 4.71 | G1.5IV-VFe-1 | 4.9 | 146.6 | D:B, 13.4v at 29". C, 12.1v at 42" and D, optical.,G:Epsilon Ind group. | |||
HR 1732 | BD+33 1008 | 34452 | 57884 | IQ Aur | 05 19 00.0 | +33 44 54 | 5.41 | A0pSi v | D:Possible CPM with HR 1728.,S:Magnetic star showing chlorine. Silicon star. Helium and neon deficient. Bluest known peculiar A-star: color,S:characteristic of about B4V. Classified A0p because He weak, but in other respects the color is more indicative of the,S:temperature than the spectral class of Ap stars. One of the hottest Ap stars known, about 17000K.,SB:Double lines.,VAR:Alpha CV 5.35 - 5.41V, 2.4660d. Spectrum var. same period. | ||||||||
HR 1733 | BD+44 1170 | 34498 | 40242 | 05 20 02.3 | +44 25 32 | 6.62 R | K0 | ||||||||||
HR 1734 | 18 | BD+33 1010 | 34499 | 57893 | 3893 | 05 19 23.6 | +33 59 08 | 6.49 | A7V | 5.3 | 3.8 | ||||||
HR 1736 | BD+46 998 | 34533 | 40251 | 3903 | 05 20 39.3 | +46 57 50 | 6.54 | GIII+A2V | 2.9 | 23.2 | D:Fixed. Companion spectral class A. | ||||||
HR 1738 | BD+40 1253 | 34557 | 40248 | 05 20 14.8 | +41 05 10 | 5.52 | A3V | ||||||||||
HR 1740 | 19 | BD+33 1013 | 34578 | 57906 | 2399 | 1925 | 05 20 00.9 | +33 57 29 | 5.03 | A5II | |||||||
HR 1749 | ρ | 20 | BD+41 1162 | 34759 | 40269 | 2400 | 05 21 48.4 | +41 48 16 | 5.23 | B3V | G:Cas-Tau OB1.,SB:35.5d, K 28k/s, V0 +19k/s, asini 13.7. | ||||||
HR 1752 | BD+29 869 | 34790 | 77124 | 05 21 12.7 | +29 34 12 | 5.76 R | A1V s | 0.4 | 0.0 | SB:6.2, 6.6v, sep. 0.0005", 2.1517d, K 113.3k/s, V0 -19.7k/s, msin3i 1.71, asini 3.35; vsini both components 53k/s. | |||||||
HR 1760 | BD+40 1268 | 34904 | 40290 | 05 22 50.3 | +41 01 46 | 5.54 | A3V | ||||||||||
HR 1768 | 22 | BD+28 788 | 35076 | 77139 | 05 23 22.9 | +28 56 12 | 6.46 | B9V s | |||||||||
HR 1773 | σ | 21 | BD+37 1175 | 35186 | 57981 | I | 3984 | 05 24 39.2 | +37 23 08 | 4.99 | K4III | 7.0 | 8.7 | D:AB fixed. | |||
HR 1775 | BD+31 954 | 35238 | 57987 | 05 24 38.3 | +31 13 26 | 6.28 | K1III | ||||||||||
HR 1776 | BD+31 955 | 35239 | 57988 | 05 24 38.5 | +31 08 35 | 5.94 | B9III | ||||||||||
HR 1779 | BD+34 1031 | 35295 | 57999 | 4000 A | 05 25 13.0 | +34 51 19 | 6.55 | K1pIII-IV+F6V | 1.8 | 31.2 | D:CPM. Companion F6V.,S:Component A has abnormally strong CN. Lambda 4150 star. | ||||||
HR 1794 | BD+35 1102 | 35519 | 58029 | 2408 | I | 05 26 54.3 | +35 27 26 | 6.15 | K2 | G:Open cluster NGC 1907 #1. | |||||||
HR 1795 | BD+34 1040 | 35520 | 58028 | 05 26 48.9 | +34 23 30 | 5.94 | A0III | S:Also classified A1p. | |||||||||
HR 1796 | BD+33 1045 | 35521 | 58030 | 05 26 51.3 | +33 15 46 | 6.15 | K0 | ||||||||||
HR 1804 | BD+30 898 | 35600 | 58040 | 05 27 08.3 | +30 12 31 | 5.74 | B9Ib | G:Aur OB1. Concentration of hydrogen emission in direction of this association. | |||||||||
HR 1805 | φ | 24 | BD+34 1048 | 35620 | 58051 | I | W | 05 27 38.9 | +34 28 33 | 5.07 | K3IIICN+2 | 3.2 | 206.8 | G:Hyades group. | |||
HR 1822 | BD+29 909 | 35984 | 77205 | 05 29 40.6 | +29 11 11 | 6.24 | F6III | ||||||||||
HR 1824 | BD+41 1206 | 36040 | 40387 | 2412 | 05 30 48.6 | +41 27 43 | 6.00 | K0IIIp | S:Lambda 4150 star. | ||||||||
HR 1825 | BD+39 1322 | 36041 | 58129 | W | 05 30 45.1 | +39 49 33 | 6.37 | G9III | 1.3 | 75.4 | D:Companion 7.62V, +0.94(B-V), +0.69(U-B), G8III. | ||||||
HR 1843 | χ | 25 | BD+32 1024 | 36371 | 58164 | 1151 | 05 32 43.7 | +32 11 31 | 4.76 | B5Iab | G:Aur OB1. Concentration of hydrogen emission in direction of this association.,SB:655.16d, K 20.5k/s, V0 -0.2k/s, asini 182. | ||||||
HR 1846 | BD+41 1218 | 36404 | 40426 | 05 33 28.7 | +42 06 32 | 6.55 | B9IIIp:Hg: | ||||||||||
HR 1850 | BD+32 1028 | 36484 | 58179 | 05 33 27.5 | +32 48 04 | 6.48 | A2m | ||||||||||
HR 1854 | BD+34 1083 | 36499 | 58182 | 05 33 38.0 | +34 43 33 | 6.27 | A3IV | ||||||||||
HR 1866 | BD+54 914 | 36678 | 25276 | 2416 | I | 05 36 35.2 | +54 25 44 | 5.73 | M0III | ||||||||
HR 1869 | BD+47 1178 | 36719 | 40466 | 2417 | 05 36 15.9 | +47 42 55 | 6.11 | dF0 | |||||||||
HR 1884 | BD+40 1346 | 36891 | 40481 | 05 36 52.4 | +40 10 56 | 6.09 | G3Ib+F | ||||||||||
HR 1904 | BD+33 1102 | 37138 | 58263 | 05 37 45.7 | +33 33 33 | 6.33 | K0 | ||||||||||
HR 1914 | 26 | BD+30 963 | 37269 | 58280 | 4229 | 2485 | 05 38 38.1 | +30 29 33 | 5.40 | F9III+B9.5V | 0.3 | 0.2 | D:AB 6.0 G5III, 6.3 A2V, 53.2y, a = 0.135". Combined, mag., colors. C, 8.57V, +0.28(B-V), +0.09(U-B), F0V at 12",,D:physical; D, 11.5v at 33". Resolved by speckle interferometry 1983.93, sep. 0.12". | ||||
HR 1924 | BD+29 947 | 37367 | 77354 | 05 39 18.4 | +29 12 55 | 5.96 | B2IV-V | 2.0 | 0.0 | G:Cas-Tau OB1.,SB:6.2, 8.2, sep. 0.00001", about 6.5d, K 9k/s. | |||||||
HR 1925 | BD+53 934 | 37394 | 25319 | W | 05 41 20.3 | +53 28 52 | 6.23 | K1V | 2.8 | 688.0 | D:Component B, 9.9v M1 at 99", is BD +53d935, CPM. Component D is F5. Other companions 12.4 and 12.8v. | ||||||
HR 1938 | BD+31 1048 | 37519 | 58319 | 2425 | 2537 | 05 40 35.9 | +31 21 29 | 6.04 | B9.5III-IVp: | ||||||||
HR 1939 | BD+31 1049 | 37536 | 58322 | I | NO Aur | 05 40 42.1 | +31 55 15 | 6.11 | M2IIIS | G:Aur OB1.,VAR:Lc 6.13 - 6.30V. | |||||||
HR 1945 | BD+29 953 | 37646 | 77393 | 4262 A | 05 41 21.0 | +29 29 15 | 6.43 | B8IV | 0.4 | 26.1 | D:CPM, B is 7.18V, -0.04(B-V), -0.14(U-B), B9.5V, vsini 120k/s.,SB:ADS 4254A. | ||||||
HR 1971 | ο | 27 | BD+49 1398 | 38104 | 40583 | 216 | 05 45 54.0 | +49 49 35 | 5.47 | A2VpCr | G:UMa stream. | ||||||
HR 1974 | BD+40 1403 | 38189 | 40584 | 05 45 49.5 | +40 30 26 | 6.58 | A3Del Del | ||||||||||
HR 1979 | BD+42 1396 | 38358 | 40609 | 2431 | 05 47 14.7 | +42 31 36 | 6.29 | K0 | |||||||||
HR 1995 | τ | 29 | BD+39 1418 | 38656 | 58465 | I | 4398 | 05 49 10.5 | +39 10 52 | 4.52 | G8IIIFe-1 | 6.1 | 49.6 | G:Ursa cluster? UMa stream. | |||
HR 2003 | BD+51 1117 | 38765 | 25411 | 2437 | 05 50 56.4 | +51 30 53 | 6.29 | K1III | |||||||||
HR 2011 | υ | 31 | BD+37 1336 | 38944 | 58496 | 2440 | I | 2661 | 05 51 02.4 | +37 18 20 | 4.74 | M0+III-IIIbFe-0.5 | VAR:Amp. 0.1V. Cycles 35-36d in 1970-1 not confirmed in other seasons. | ||||
HR 2012 | ν | 32 | BD+39 1429 | 39003 | 58502 | 221 | I | 4440 | 05 51 29.4 | +39 08 55 | 3.97 | G9.5III* | 7.3 | 54.6 | D:Companion optical.,S:G9.5III CN 0.5 Fe 1 Ba 0.2: | ||
HR 2018 | BD+32 1109 | 39045 | 58504 | I | 4443 | Var | 05 51 25.7 | +32 07 30 | 6.25 | M3III v | 5.9 | 15.2 | M:High space velocity.,S:Spectrum may be variable.,VAR:Amp. 0.10V. | ||||
HR 2025 | BD+39 1435 | 39182 | 58524 | 05 52 39.5 | +39 34 28 | 6.45 R | A2V | ||||||||||
HR 2028 | BD+33 1179 | 39225 | 58528 | 2443 | I | 2681 | 05 52 40.1 | +33 55 03 | 5.98 | M1.5II-III | M:High space velocity. | ||||||
HR 2029 | ξ | 30 | BD+55 1027 | 39283 | 25450 | 1157 | 05 54 50.8 | +55 42 25 | 4.99 | A2V | G:Sirius group?,N:Flamsteed also called this star 32 Cam = 30 Aur.,R:Radius relative to Sun = 2.6.,S:Lambda Boo type. | ||||||
HR 2045 | BD+51 1128 | 39551 | 25467 | 05 56 14.4 | +51 48 14 | 6.49 R | A5V | ||||||||||
HR 2046 | BD+31 1139 | 39586 | 58569 | 05 54 59.0 | +31 42 06 | 5.90 | A5IV | ||||||||||
HR 2054 | BD+49 1423 | 39743 | 40720 | 05 57 04.9 | +49 01 46 | 6.47 | G8III | ||||||||||
HR 2066 | BD+28 952 | 39866 | 77744 | 05 56 33.8 | +28 56 32 | 6.32 | A2II | ||||||||||
HR 2077 | δ | 33 | BD+54 970 | 40035 | 25502 | 225 | I | W | 05 59 31.6 | +54 17 05 | 3.72 | K0-III | 5.8 | 115.4 | |||
HR 2079 | BD+55 1036 | 40062 | 25504 | 05 59 45.7 | +55 19 15 | 6.44 | A5m | ||||||||||
HR 2080 | BD+54 971 | 40083 | 25505 | 05 59 48.1 | +54 32 50 | 6.14 | K2III | ||||||||||
HR 2081 | BD+49 1428 | 40084 | 40743 | 05 59 21.8 | +49 55 28 | 5.89 | G5III | SB:219.13d, K1 32.2k/s, K2 33.23k/s, V0 -4.09k/s, a1sini 97.1, a2sini 100.1. | |||||||||
HR 2088 | β | 34 | BD+44 1328 | 40183 | 40750 | 227 | I | 4556 | Bet Aur | 05 59 31.7 | +44 56 51 | 1.90 | A2IV | 8.9 | 184.6 | D:AB binary. C, 14.1v at 13".,G:In Ursa cluster; Sirius group; UMa stream; UMa cluster.,N:Menkalinan; Menkalina.,R:Radius relative to Sun = 3.0.,SB:ADS 4556A, 3.9600d, K 107.5k/s, V0 -17.1k/s, msin3i 2.20, asini 5.85. Masses 2.33, 2.25 solar. Rotational,SB:velocities both components <30k/s. Second SB ever discovered, by Antonia Maury, 1889.,VAR:ADS 4556A, EA 1.89 - 1.98V, 1.93 - 2.02B, A2+A2, 3.9600421d, i 78.5d. | |
HR 2091 | π | 35 | BD+45 1217 | 40239 | 40756 | I | Pi Aur | 05 59 56.1 | +45 56 13 | 4.26 | M3II e | C:Large infrared excess.,M:Radio star.,S:Ultraviolet FeII emission.,VAR:Lc 4.24 - 4.34V. Radio emission at 2.85cm indicates mass loss. | |||||
HR 2095 | θ | 37 | BD+37 1380 | 40312 | 58636 | I | 4566 | The Aur | 05 59 43.3 | +37 12 45 | 2.62 | A0pSi | 4.5 | 3.5 | D:AB binary , combined mag., colors. B is 7.2v G2V. C, 11v at 49" optical.,DYN:0.032".,R:Radius 3.3 solar.,VAR:ADS 4566B. Alpha CV 2.62 - 2.70V. Amp. 0.43m at 1400A, 1.3735d. Magnetic field varies 3.618d. | ||
HR 2096 | BD+44 1332 | 40325 | 40769 | 4576 | 06 00 19.0 | +44 35 31 | 6.22 | K2III+K0III | 4.0 | 34.2 | D:AB probably binary. B, 11v at 2". Component C, K0III, optical. | ||||||
HR 2101 | 36 | BD+47 1227 | 40394 | 40778 | 06 00 58.6 | +47 54 07 | 5.73 | B9.5pSiFe | |||||||||
HR 2105 | BD+48 1333 | 40486 | 40789 | 2458 | I | 06 01 43.1 | +48 57 34 | 5.96 | K0 | ||||||||
HR 2110 | BD+31 1164 | 40588 | 58657 | 06 01 10.2 | +31 02 05 | 5.98 R | A2V | ||||||||||
HR 2112 | BD+49 1441 | 40626 | 40801 | 06 02 48.7 | +49 54 20 | 6.05 | B9.5IV | ||||||||||
HR 2115 | BD+43 1421 | 40722 | 40808 | 06 02 53.6 | +43 22 43 | 6.42 R | K0 | ||||||||||
HR 2119 | 38 | BD+42 1473 | 40801 | 40818 | 2461 | 06 03 18.0 | +42 54 42 | 6.10 | K0II | G:Sigma Pup group. | |||||||
HR 2122 | BD+32 1166 | 40832 | 58688 | 06 02 55.1 | +32 38 09 | 6.24 | F4V | ||||||||||
HR 2123 | BD+51 1146 | 40873 | 25548 | 2463 | 4633 | 2804 | 06 04 29.1 | +51 34 24 | 6.45 | A7III | 2.8 | 39.0 | D:BC, 9.0, 10.0v, sep. 0.6", CPM with A.,VAR:Delta Sct? | ||||
HR 2132 | 39 | BD+42 1477 | 41074 | 40840 | 2812 | 06 05 03.4 | +42 58 54 | 5.87 | F3V | G:Hyades group. | |||||||
HR 2137 | BD+37 1405 | 41162 | 58716 | 4649 | 06 05 02.6 | +37 57 51 | 6.34 | K0III+A2 | 5.6 | 17.9 | D:Confusion as to whether B or C is the brighter, B at 18", C at 84" from A. | ||||||
HR 2139 | BD+33 1236 | 41269 | 58727 | 06 05 34.0 | +33 35 57 | 6.23 | B9pSi | ||||||||||
HR 2141 | BD+35 1334 | 41330 | 58739 | W | 06 06 08.5 | +35 23 15 | 6.12 | G0V | 3.4 | 122.0 | |||||||
HR 2143 | 40 | BD+38 1377 | 41357 | 58749 | 2465 | Var? | 06 06 35.1 | +38 28 58 | 5.36 | A4m | SB:28.28d, K 51.4k/s, V0 +16.9k/s, msin3i 1.35, asini 16.6.,VAR:Suspected of 0.01m variability. | ||||||
HR 2146 | BD+29 1112 | 41429 | 77958 | I | 4673 | 06 06 22.5 | +29 30 45 | 6.08 | M3II+F7V | 5.0 | 10.0 | D:CPM. Companion 10.72V, +0.90(B-V), +0.25(U-B), F7V. | |||||
HR 2147 | BD+41 1357 | 41467 | 40868 | 06 07 26.9 | +41 51 15 | 6.12 | K0III | ||||||||||
HR 2153 | BD+41 1365 | 41636 | 40881 | 06 08 23.0 | +41 03 20 | 6.36 | G9III | ||||||||||
HR 2172 | BD+52 1041 | 42083 | 25613 | 06 11 46.0 | +52 38 50 | 6.30 | A5IIIm | SB:106d, K 40.5k/s, V0 +13.5k/s, msin3i 1.55, asini 45.8; vsini both components 30k/s. Unresolved by speckle,SB:interferometry. | |||||||||
HR 2175 | 41 | BD+48 1352 | 42126 | 40924 | 4773 B | 06 11 36.5 | +48 42 47 | 6.82 H | A8V | 0.8 | 7.7 | D:Binary with HR 2176.,G:Hyades group. | |||||
HR 2176 | 41 | BD+48 1352 | 42127 | 40925 | 4773 A | 06 11 36.6 | +48 42 40 | 6.09 H | A3V | 0.8 | 7.7 | D:Binary with HR 2175.,G:Hyades group. | |||||
HR 2188 | BD+51 1163 | 42466 | 25630 | 06 13 45.3 | +51 10 21 | 6.04 | K1III | ||||||||||
HR 2189 | BD+32 1217 | 42471 | 58852 | 2470 | I | 06 12 20.1 | +32 41 36 | 5.78 | M2IIIa | ||||||||
HR 2217 | BD+36 1388 | 43017 | 58905 | 1167 | 4849 A | 06 15 39.0 | +36 08 55 | 6.92 | F4IV | 0.6 | 11.3 | D:AB CPM. B is dF0; C 12.3v at 202" optical. D, 11.5v at 120" from A. | |||||
HR 2219 | κ | 44 | BD+29 1154 | 43039 | 78143 | 1168 | I | 2877 | 06 15 22.7 | +29 29 53 | 4.35 | G8.5IIIb | |||||
HR 2228 | 42 | BD+46 1122 | 43244 | 40999 | 06 17 34.7 | +46 25 27 | 6.52 | F0V | G:UMa stream. | ||||||||
HR 2239 | 43 | BD+46 1124 | 43380 | 41010 | 06 18 16.9 | +46 21 38 | 6.38 | K2III | G:Eta Cep group. | ||||||||
HR 2264 | 45 | BD+53 1008 | 43905 | 25681 | 2484 | 06 21 46.1 | +53 27 08 | 5.36 | F5III | SB:6.5013d, K 31.7k/s, V0 -1.5k/s, asini 2.83. | |||||||
HR 2272 | BD+29 1190 | 44092 | 78259 | 06 21 12.1 | +29 32 28 | 6.43 | A1V s | ||||||||||
HR 2289 | ψ1 | 46 | BD+49 1488 | 44537 | 41076 | 242 | I | Psi1 Aur | 06 24 53.9 | +49 17 17 | 4.91 | K5-M0Iab-Ib | VAR:Lc? 4.75 - 5.70V, 6.6 - 7.2p. | ||||
HR 2297 | BD+29 1213 | 44766 | 78333 | 06 24 52.6 | +29 42 26 | 6.71 | B8IIIn | ||||||||||
HR 2314 | BD+47 1299 | 45105 | 41109 | 06 27 51.1 | +47 24 19 | 6.56 | A0V | ||||||||||
HR 2319 | BD+32 1300 | 45192 | 59096 | 06 27 35.5 | +32 33 47 | 6.43 | K0 | ||||||||||
HR 2332 | 48 | BD+30 1238 | 45412 | 59128 | RT Aur | 06 28 34.1 | +30 29 35 | 5.55 | F8Ib v | S:Also classified F4Ib-G1Ib.,VAR:CDelta 5.02 - 5.82V. Per. changing, 3.728365 before 1950, 3.728115 since. CaII emission on rising branch of light,VAR:curve. Blue companion suspected. | |||||||
HR 2338 | 47 | BD+46 1149 | 45466 | 41130 | 2496 | I | 06 30 03.0 | +46 41 08 | 5.90 | gK4 | |||||||
HR 2372 | BD+32 1324 | 46052 | 59194 | 2500 | WW Aur | 06 32 27.2 | +32 27 17 | 5.87 | A3m+A3m: | S:Also classified A3m: + A3m:,SB:2.5250d, K 115.6k/s, V0 -8.7k/s, msin3i 1.98, asini 4.01. Masses 1.92, 1.90 solar. vsini same for both,SB:components 35k/s.,VAR:EA 5.79 - 6.54V, 2.52501922d. Per. changes. Rot. line apsides per. about 40,000d. | |||||||
HR 2383 | BD+33 1356 | 46251 | 59222 | 06 33 42.7 | +33 01 27 | 6.42 R | A3V | ||||||||||
HR 2398 | 49 | BD+28 1168 | 46553 | 78524 | 2504 | 3032 | 06 35 12.1 | +28 01 20 | 5.27 | A0Vnn | |||||||
HR 2405 | BD+38 1539 | 46687 | 59280 | I | W | UU Aur | 06 36 32.9 | +38 26 43 | 5.29 | C5II | 5.6 | 17.9 | S:Infrared spectra show CO, CN and C2 molecules.,VAR:SRb 7.83 - 10.00B, 8.2 - 10.0p, 234d. Mean mag. varies in per. about 3500d. | ||||
HR 2419 | 51 | BD+39 1690 | 47070 | 59316 | 250 | I | 06 38 39.5 | +39 23 27 | 5.69 | K5III | G:Hyades group. | ||||||
HR 2420 | ψ3 | 52 | BD+40 1665 | 47100 | 59319 | 06 38 49.2 | +39 54 09 | 5.20 | B8III | ||||||||
HR 2425 | 53 | BD+29 1293 | 47152 | 78571 | D | 06 38 23.0 | +28 59 03 | 5.79 | B9npEu | 0.0 | 0.1 | D:Discovered by both occultation and speckle interferometry 1978, sep. 0.075"; 1983.93, sep. 0.13".,S:Spectra show Hg 4077; Eu, Cr enhanced. Overabundant elements are V by factor of 300; Sr by 1500; Y by 100 and rare,S:earths by hundreds of thousands. | |||||
HR 2427 | ψ2 | 50 | BD+42 1585 | 47174 | 41239 | I | W | 06 39 19.9 | +42 29 20 | 4.79 | K3III | 5.5 | 52.1 | ||||
HR 2434 | BD+44 1506 | 47270 | 41245 | 06 39 58.0 | +44 00 50 | 6.41 R | K1III | ||||||||||
HR 2438 | 54 | BD+28 1196 | 47395 | 78593 | 5289 | 3065 | 06 39 33.1 | +28 15 47 | 6.03 | B7III | 1.6 | 0.8 | |||||
HR 2452 | BD+36 1482 | 47703 | 59365 | 2516 | 06 41 37.7 | +35 55 55 | 6.46 | F8III | |||||||||
HR 2459 | ψ4 | 55 | BD+44 1518 | 47914 | 41288 | 2517 | I | 06 43 05.0 | +44 31 28 | 5.02 | K5III | ||||||
HR 2464 | BD+37 1567 | 48073 | 59406 | 06 43 13.8 | +37 08 49 | 6.19 | K0 | ||||||||||
HR 2471 | BD+36 1494 | 48272 | 59425 | 06 44 12.6 | +36 06 35 | 6.31 R | A2V | ||||||||||
HR 2483 | ψ5 | 56 | BD+43 1595 | 48682 | 41330 | 255 | 5425 | 06 46 44.3 | +43 34 39 | 5.25 | G0V | 3.4 | 36.2 | D:Companion orange, optical. | |||
HR 2487 | ψ6 | 57 | BD+48 1436 | 48781 | 41346 | 1176 | I | 06 47 39.6 | +48 47 22 | 5.22 | K0III | ||||||
HR 2516 | ψ7 | 58 | BD+41 1536 | 49520 | 41380 | 2527 | I | W | 06 50 45.9 | +41 46 53 | 5.02 | K3III | 5.0 | 40.9 | G:61 Cyg group. | ||
HR 2532 | BD+45 1359 | 49949 | 41406 | 06 53 07.6 | +44 50 22 | 6.26 | A8Vn | ||||||||||
HR 2539 | 59 | BD+39 1771 | 50018 | 59571 | 5534 | OX Aur | 06 53 01.5 | +38 52 09 | 6.12 | F2VDel Del v | 3.9 | 22.3 | D:AB fixed.,M:Space motion almost identical to that of the Sun.,S:Also classified A7n-F3IV.,VAR:Delta Sct 5.94 - 6.14V, primary period 0.115442, secondary 0.154412d. | ||||
HR 2541 | 60 | BD+38 1636 | 50037 | 59576 | S | 06 53 13.4 | +38 26 17 | 6.30 | dF5 | N:Sometimes this star, sometimes HR 2547 have been called Psi8 Aur. To avoid future confusion this designation,N:is abandoned for both. | |||||||
HR 2542 | BD+35 1511 | 50056 | 59574 | I | 3250 | 06 53 03.4 | +35 47 19 | 6.01 | K3III: | ||||||||
HR 2547 | ψ8 | 61 | BD+38 1638 | 50204 | 59589 | 06 53 57.0 | +38 30 18 | 6.48 | B9.5pSi | N:See note for HR 2541.,S:Hg, Mn. | |||||||
HR 2556 | BD+46 1202 | 50384 | 41426 | 06 55 15.2 | +45 49 35 | 6.34 | K0III-IV | G:Hyades group. | |||||||||
HR 2557 | BD+44 1551 | 50420 | 41429 | V352 Aur | 06 55 14.7 | +43 54 36 | 6.13 | A9III | VAR:Delta Sct 6.037 - 6.054y. About 4 hrs. One of most luminous Delta Sct stars: abs. mag. about 0.0V. | ||||||||
HR 2568 | ψ9 | BD+46 1203 | 50658 | 41446 | Var? | 06 56 32.3 | +46 16 27 | 5.87 | B8IIIe | S:Shell star.,VAR:Emission var. about 16 yrs. | |||||||
HR 2573 | BD+46 1205 | 50763 | 41450 | 06 56 56.0 | +46 42 18 | 5.86 | gK0 | ||||||||||
HR 2600 | 62 | BD+38 1656 | 51440 | 59658 | 2538 | I | 06 59 02.8 | +38 03 08 | 6.00 | K2III | |||||||
HR 2675 | BD+37 1660 | 53925 | 59812 | 07 08 36.3 | +37 26 42 | 6.16 | K1III | ||||||||||
HR 2696 | 63 | BD+39 1882 | 54716 | 59866 | 274 | I | 07 11 39.3 | +39 19 14 | 4.90 | K4III-IIIa | |||||||
HR 2753 | 64 | BD+41 1630 | 56221 | 41679 | 276 | 07 18 02.2 | +40 53 00 | 5.78 | A5Vn | G:In Ursa cluster? | |||||||
HR 2775 | BD+42 1699 | 56941 | 41705 | 07 21 03.1 | +42 39 20 | 6.35 | K0 | ||||||||||
HR 2792 | BD+39 1927 | 57263 | 60012 | 07 22 13.4 | +38 59 46 | 6.40 | K0 | ||||||||||
HR 2793 | 65 | BD+37 1707 | 57264 | 60010 | 2568 | I | 6009 | 07 22 02.6 | +36 45 38 | 5.13 | K0III | 5.5 | 11.4 | D:AB CPM. C, 12.7v at 42" optical. | |||
HR 2805 | 66 | BD+40 1852 | 57669 | 41738 | 1191 | I | 07 24 08.5 | +40 40 20 | 5.19 | K1+IIIaCN1 |
Planetary Nebulae | ||||||||
---|---|---|---|---|---|---|---|---|
Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
NGC 2242 | 06 34 07.4 | +44 46 40 | PN | 15.1 | 15.0 | 0.37 | eeF, vS, R, F * nf | PK 170+15.1, CGCG 204-5 |
IC 2149 | 05 56 23.9 | +46 06 19 | PN | 11.2 | 10.6 | 0.57 | Planetary, stellar | PK 166+10.1, CS=10.5 |
Galactic Nebulae | ||||||||
Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
NGC 1931 | 05 31 25.7 | +34 14 42 | EN+OCL | 10.1 | vB, L, R, B *** in M | LBN 810, OCL 441 | ||
NGC 1985 | 05 37 47.8 | +31 59 20 | RN | 12.7 | 0.68 | cF, S, R, psbM | PK 176+0.1, CS=13.6, not a PN | |
IC 405 | 05 16 29.4 | +34 21 22 | EN | 10.0 | 30 × 20 | * 6.7 with pB, vL neb | LBN 795, CED 42, in Sh2-229 (Flaming Star nebula) | |
IC 410 | 05 22 45.0 | +33 24 48 | EN+OCL | 55 × 45 | Dif, many st inv | LBN 807, OCL 439, around NGC1893 | ||
IC 417 | 05 28 05.9 | +34 25 26 | EN+OCL | 13 × 10 | vL, dif, * 6 inv | LBN 804, CED 46, Sh2-234 | ||
Open Clusters | ||||||||
Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
NGC 1664 | 04 51 05.4 | +43 40 34 | III1p | 7.6 | 18 | Cl, lRi, lC, pL | OCL 411 | |
NGC 1778 | 05 08 05.0 | +37 01 24 | III2p | 7.7 | 8 | Cl, pC, lRi, iF, st L | OCL 429 | |
NGC 1798 | 05 11 39.3 | +47 41 44 | II2m | 10.0 | 5 | S, Cl or Cl + neb | OCL 410, Berkeley 16 | |
NGC 1857 | 05 20 05.0 | +39 20 36 | II2m | 7.0 | 10 | Cl, pRi, pC, st 7… | OCL 428 | |
NGC 1883 | 05 25 54.1 | +46 29 25 | II3p | 12.0 | 5 | Cl, vF, pRi, pC, iF | OCL 417 | |
NGC 1893 | 05 22 45.6 | +33 24 52 | II2mn | 7.5 | 10 | Cl, L, Ri, lC | OCL 439, in IC 410, LBN 807 | |
NGC 1907 | 05 28 04.5 | +35 19 32 | II1m | 8.2 | 5 | Cl, pRi, pC, R, st 9…12 | OCL 434 | |
NGC 1912 | 05 28 43.0 | +35 51 18 | II2r | 6.4 | 15 | Cl, B, vL, vRi, iF, st L & S | M 38, OCL 433 | |
NGC 1960 | 05 36 17.7 | +34 08 27 | II3m | 6.0 | 10 | Cl, B, vL, vRi, lC, st 9…11 sc | M 36, OCL 445 | |
NGC 2013 | 05 44 01.6 | +55 47 22 | OCL | Cl, vlRi, st 11 | ||||
NGC 2099 | 05 52 18.3 | +32 33 11 | II1r | 5.6 | 15 | Cl, Ri, pCM, st L & S | M 37, OCL 451 | |
NGC 2126 | 06 02 32.9 | +49 51 57 | II1p | 10.2 | 6 | Cl, not Ri, * 7 m north | OCL 418 | |
NGC 2165 | 06 11 04.0 | +51 40 42 | OCL | 13.4 | 12.7 | 6 | Cl, pL, poor, st 11 | |
NGC 2192 | 06 15 17.4 | +39 51 19 | III1p | 10.9 | 5 | Cl, cL, C, iF, st vS | OCL 437 | |
NGC 2240 | 06 33 10.5 | +35 15 02 | OCL | Cl, pL, P, vlC, st 7, 10…15 | ||||
NGC 2281 | 06 48 17.8 | +41 04 44 | I3p | 5.4 | 25 | Cl, pRi, vlC, st pL | OCL 446 | |
Galaxies | ||||||||
Name | RA | Dec | Type | bMag | vMag | Dim | Dreyer Description | Identification, Remarks |
NGC 2208 | 06 22 34.6 | +51 54 36 | S0 | 13.8 | 12.8 | 1.6 × 1.1 | pF, pS, lE | UGC 3452, MCG 9-11-10, CGCG 260-7, NPM1G +51.0053 |
NGC 2303 | 06 56 17.4 | +45 29 36 | E0 | 13.6 | 12.6 | 1.5 × 1.5 | eF, vS, R, sev st nr | UGC 3603, MCG 8-13-31, CGCG 234-30, NPM1G +45.0083 |
IC 2190 | 07 29 54.3 | +37 27 06 | SBbc | 14.8 | 14.0 | 0.9 × 0.5 | F, pS, dif | UGC 3880, MCG 6-17-13, CGCG 177-26 |
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 G158.9+17.8 | 06 19 34 | +55 36 43 | PuWe 1 | PURGATHOFER et al 1980 | 1200. | 27.0 (O-III), 27.0 (N-II) | AG82 61 | B: 15.3 | sd O | ||||||
PN G163.1-00.8 | 04 54 31 | +42 16 37 | We 1- 3 | WEINBERGER 1977 | 115. | AG82 37 | U: 20.23, B: 21.24, V: 21.01 | ||||||||
PN G166.1+10.4 | 05 56 24 | +46 06 17 | IC 2149 | 166+10.1 | 05526+4605 | FLEMING 1906 | ARO 23, VV 26, VV' 37 | 8.5 | 7. | 1.09 | -30.7 ± 2.1 | < 10.0 (O-III), 20. (N-II) | AG82 51, BD +46 1067, GCRV 3681, HD 39659, PLX 1357 | B: 11.28, V: 11.59 | O4 (f), Of(H) |
PN G166.4-06.5 | 04 42 53 | +36 06 53 | CRL 618 | 04395+3601 | WESTBROOK et al 1975 | 12. | 1.0 | AFGL 618, AG82 35 | V: 17.0 | BO - O9.5 ? | |||||
PN G167.0-00.9 | 05 06 38 | +39 08 08 | A 8 | 167-00.1 | ABELL 1955 | A55 7, ARO 216, VV' 28 | 60. | +58.2 ± 6.5 | AG82 40 | B: 20.2 | |||||
PN G170.3+15.8 | 06 34 07 | +44 46 38 | NGC 2242 | 06304+4448 | SHAW et al 1987 | 22. | B: 17.4, V: 17.6 | ||||||||
PN G170.7+04.6 | 05 41 22 | +39 15 08 | K 3-69 | 05378+3913 | KOHOUTEK 1969 | 0. | 0.45 | +22.9 ± 4.0 | |||||||
PN G173.5+03.2 | 05 42 34 | +36 09 05 | Pu 2 | PURGATHOFER 1980 | 20. | +45.0 ± 5.2 | AG82 55 | B: 20.9, V: 19.9 | |||||||
PN G173.7+02.7 | 05 40 53 | +35 42 35 | PP 40 | TURNER et al 1985 | GM 1-66 | 30. : | 30. | ||||||||
PN G173.7-05.8 | 05 07 09 | +30 50 03 | K 2- 1 | 173-05.1 | KOHOUTEK 1963 | ARO 175 | 132. | +19.2 ± 4.5 | AG82 41 | B: 18.8 | |||||
PN G178.3-02.5 | 05 31 36 | +28 58 41 | K 3-68 | 05284+2856 | KOHOUTEK 1969 | We 2-21 | 10. | 12. | +65.0 ± 4.8 | AG82 45 | |||||
PN G183.8+05.5 | 06 16 11 | +28 22 05 | WeSb 2 | WEINBERGER et al 1981 | 135. |
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) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Pal 2 | 04 46 05.91 | +31 22 53.4 | 27.2 | 35.0 | -1.42 | 1 | 1.24 | 21.60 | 21.01 | 13.04 | -7.97 | 1.83 | 2.08 | 2.65 | 0.05 | -133.0 ± 57.0 | -140.1 | 1.53 | 0.17 | 0.50 | 19.06 | 4.06 | 8.82 | 9.28 |