Kataloge

Lacerta / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HR B F DM HD SAO FK5 IR M* ADS VarID RA Dec vMag spType dMag Sep Remarks
HR 8421 BD+46 3574 209857 51632 I HT Lac 22 05 16.4 +46 44 41 6.13 M4IIIab G:NGC 7209 #86.,VAR:SRb 6.08 - 6.36V, 82:d.
HR 8422 BD+44 4041 209932 51640 22 05 50.6 +45 06 44 6.44 A0V
HR 8424 BD+44 4043 209945 51650 3769 I 14028 22 06 02.0 +45 00 52 5.14 K5III
HR 8427 BD+47 3692 209961 51645 V365 Lac 22 05 51.2 +48 13 54 6.27 B2V G:Lac OB1.,SB:2.1727d, K 121.7k/s, V0 -12.9k/s, asini 3.63. Secondary black hole? Masses 12 and over 5 solar.,VAR:Amp. 0.08V, 2.1727d.
HR 8429 BD+44 4044 209993 51652 22 06 12.4 +45 14 55 6.19 A3V
HR 8443 BD+52 3114 210221 34076 22 07 25.5 +53 18 26 6.14 A3Ib
HR 8445 BD+49 3746 210289 51678 I 15659 22 08 16.5 +49 47 47 6.42 R K5III 6.7 38.5
HR 8448 BD+45 3813 210334 51684 AR Lac 22 08 41.0 +45 44 31 6.11 G2IV+K0III S:Published classes range from F8, G2IV, G2Vn to G5IV for the earlier component, and K0IV to K2III for the later. Radio,S:emission source probably synchrotron emission.,SB:1.9832d, K 116.1k/s, V0 -33.7k/s, msin3i 1.28, asini 3.17. Masses 1.2 and 1.3 solar. Mass loss from primary.,SB:Close radio binary.,VAR:EA 6.08 - 6.77V, RS CVn-type binary, 1.98319204d (period changes). Distortions in light curve possibly due to star,VAR:spots or to gas streams. Strong radio flare activity.
HR 8463 BD+50 3602 210715 34143 3774 15708 22 11 09.9 +50 49 24 5.40 A5V 4.1 73.8 D:B and C optical. D, K0, CPM.
HR 8485 BD+38 4711 211073 72155 1583 I 15758 14076 22 13 52.7 +39 42 54 4.49 K3III 6.3 28.4 D:B, optical.,G:In reflection nebula.,SB:ADS 15758A. Resolved by speckle interferometry 1983.94, sep. 0.09".
HR 8487 BD+44 4073 211096 51783 22 13 49.3 +45 26 27 5.53 A0III
HR 8489 BD+42 4333 211211 51797 3778 22 14 44.4 +42 57 14 5.71 A2Vnn
HR 8498 1 BD+37 4526 211388 72191 I 22 15 58.2 +37 44 56 4.13 K3-II-III
HR 8510 BD+37 4537 211797 72228 15828 22 18 56.2 +37 46 10 6.17 A9IIIp 2.7 15.7 D:AB binary.
HR 8519 BD+50 3673 212071 34335 22 20 39.6 +50 58 51 6.42 R K2
HR 8523 2 BD+45 3894 212120 51904 15862 14130 22 21 01.6 +46 32 12 4.57 B6V 6.4 48.2 D:Visual companion is optical.,SB:ADS 15862A, 2.6164d, K 79.5k/s, V0 -8.9k/s, msin3i 0.873, asini 2.86. Secondary about 1m fainter.,VAR:ADS 15862A, Ell?, 4.53 - 4.56V.
HR 8528 BD+41 4469 212222 51918 22 21 50.9 +42 04 42 6.41 B5V
HR 8536 BD+37 4560 212487 72296 22 23 54.2 +38 34 25 6.22 F5IV:
HR 8538 β 3 BD+51 3358 212496 34395 844 I S 22 23 33.6 +52 13 45 4.43 G8.5IIIbCa1
HR 8541 4 BD+48 3715 212593 51970 22 24 31.0 +49 28 35 4.57 B9Iab
HR 8549 BD+36 4835 212883 72344 15942 22 26 45.7 +37 26 38 6.46 B2V 3.3 4.3 D:Fixed.,G:Lac OB1.
HR 8553 BD+39 4841 212978 72358 S 22 27 26.5 +39 48 35 6.14 B2V 0.2 G:Lac OB1.
HR 8554 BD+55 2750 212986 34460 3795 22 26 59.2 +56 26 00 6.57 B5III
HR 8569 BD+34 4700 213272 72399 22 29 43.9 +35 43 32 6.56 A2V
HR 8572 5 BD+46 3719 213310 52055 3799 I S 14177 22 29 31.8 +47 42 25 4.36 M0II+B8V SB:41.95y, K 12.2k/s, V0 -3.4k/s, asini 2240. Unresolved by speckle interferometry. SKYLAB indicates cool star with,SB:hot companion. vsini of B-type component 90:k/s.
HR 8575 BD+48 3747 213389 52073 W V350 Lac 22 30 06.5 +49 21 22 6.40 K2IIIe 3.2 66.0 S:Strong CaII emission.,SB:17.755d, K 40.2k/s, V0 +5.4k/s, asini 9.81.,VAR:Ell 6.27 - 6.47V, 17.748d, double wave light curve; mean mag. varies.
HR 8579 6 BD+42 4420 213420 52079 3800 22 30 29.3 +43 07 24 4.51 B2IV G:Lac OB1.,SB:880d, K 9k/s, V0 -11.9k/s, asini 104.
HR 8585 α 7 BD+49 3875 213558 34542 848 16021 22 31 17.5 +50 16 57 3.77 A1V 8.3 36.3 D:Optical.
HR 8588 BD+39 4871 213660 72446 3805 16031 22 32 26.4 +39 46 47 5.88 A6V 5.5 43.1
HR 8589 BD+53 2910 213720 34555 22 32 18.8 +54 02 15 6.35 R G8III
HR 8594 BD+55 2769 213930 34574 I 14213 22 33 40.6 +56 37 30 5.71 G8III-IV VAR:L, 5.8 - 6.8v, period about 1y.
HR 8603 8 BD+38 4808 214168 72509 16095 A 14242 22 35 52.3 +39 38 03 5.73 B2Ve v 0.7 22.4 D:AB CPM. B is 6.46V, -0.14(B-V), -0.82(U-B), B2V, vsini 40k/s. All companions listed by Worley are more than 22" from,D:A. A new companion at 0.042" discovered by speckle interferometry.,G:Lac OB1.,RV:ADS 16095A, cycles 4-10y.,S:Shell star.,VAR:ADS 16095A, 4-10y cycles. Emission var. period 16-18y.
HR 8606 BD+49 3903 214240 52171 22 35 53.4 +50 04 16 6.29 B3V G:Lac OB1.,SB:10.9188d, K 82.3k/s, V0 -16.4k/s, asini 12.0. Secondary spectrum faint.
HR 8607 BD+55 2779 214279 34605 22 35 51.8 +56 04 12 6.38 A3V
HR 8609 BD+34 4729 214313 72535 3812 22 36 48.7 +35 39 09 6.30 K5
HR 8613 9 BD+50 3770 214454 34628 22 37 22.4 +51 32 43 4.63 A8IV
HR 8617 BD+44 4185 214558 52211 S 22 38 17.5 +45 10 59 6.40 R G2III+A4V 0.1 S:vsini of both components =<50k/s.
HR 8621 BD+56 2821 214665 34651 I 16140 14260 22 38 37.9 +56 47 45 5.21 R M4+III 5.2 30.9 D:Optical.
HR 8622 10 BD+38 4826 214680 72575 852 16148 22 39 15.7 +39 03 01 4.88 O9V 5.2 62.2 C:Color excess E(B-V) = +0.11.,D:Companion 10.02V, +0.28(B-V), +0.3(U-B), A6III-IV, vsini 141k/s.,G:Lac OB1; in HII region.,RV:Possible rapid variations arising in outer layers of the stellar atmosphere. Probably fast rotating pole-on star.
HR 8626 BD+36 4902 214714 72581 16154 22 39 34.3 +37 35 34 6.03 G3Ib-IICN-1CH2Fe-1 5.7 19.5 D:Optical.
HR 8632 11 BD+43 4266 214868 52251 I 22 40 30.9 +44 16 35 4.46 K2+III-IIIb G:Hyades group.
HR 8633 BD+53 2950 214878 34682 22 40 18.4 +53 50 46 5.93 K0III
HR 8640 12 BD+39 4912 214993 72627 W DD Lac 22 41 28.6 +40 13 32 5.25 B2III 4.0 69.0 D:B, 9.2A3V, physical, vsini 89k/s.,G:Lac OB1.,SB:0.19d and slower var.,VAR:Beta C 5.16 - 5.28V, 0.1930924d. Six secondary periods reported, ranging from 0.095109 to 0.23583d.
HR 8643 BD+40 4885 215030 52270 22 41 36.1 +41 32 58 5.94 R G9III
HR 8648 BD+53 2960 215159 34713 3817 I 22 42 20.8 +53 54 32 6.12 K2
HR 8651 BD+37 4670 215191 72652 22 42 55.5 +37 48 10 6.43 B1V G:Lac OB1.
HR 8652 BD+46 3803 215242 52296 16214 14290 22 43 04.5 +47 10 07 6.39 A1V+G: 1.6 0.5 D:BC, 7.6, 9.5v sep. 0.15" binary and AxBC binary.,SB:ADS 16214BC.,VAR:Uncertain which component varies.
HR 8654 BD+38 4855 215359 72675 I 16228 22 44 05.2 +39 27 56 5.95 K5III+K2III 3.5 2.7 D:AB binary. B is K2III. C, 12.5v at 11" optical.,DYN:0.005".
HR 8656 13 BD+41 4594 215373 52317 858 I 16227 22 44 05.5 +41 49 09 5.08 K0III 5.8 14.6 D:Fixed sep.
HR 8661 BD+51 3460 215518 34757 I 22 44 49.2 +52 31 02 6.55 R K2
HR 8666 BD+43 4300 215664 52348 14311 22 46 10.2 +44 32 46 5.76 F0III-IV G:Hyades moving group.,VAR:Delta Sct?, amp. 0.01V, 0.052:d.
HR 8678 BD+36 4934 215943 72732 14321 22 48 10.9 +37 25 00 5.90 gG8
HR 8682 BD+53 2993 216057 34845 22 48 47.8 +54 24 54 6.12 B5Vne M:Old disk population runaway star.,S:Shell star. Also classified B8.5IV-V.
HR 8688 BD+55 2820 216174 34858 I 22 49 46.2 +55 54 10 5.43 K1III
HR 8690 14 BD+41 4623 216200 52412 S V360 Lac 22 50 21.8 +41 57 13 5.92 B3IV: e 1.0 G:Lac OB1.,S:H alpha emission.,SB:10d.,VAR:EB 5.91 - 5.98V, 10.075d. Detached main sequence stars.
HR 8692 BD+49 3954 216206 34862 22 50 10.2 +50 40 37 6.21 G4Ib
HR 8699 15 BD+42 4521 216397 52436 I 16325 22 52 02.0 +43 18 45 4.94 M0III 6.0 104.4 D:AB, CPM. B, 12.2v at 26".
HR 8705 BD+49 3962 216523 34917 22 52 52.3 +50 24 43 6.46 B8V
HR 8706 BD+39 4957 216538 72812 14346 22 53 11.3 +40 10 02 6.34 B7III-IV
HR 8708 BD+43 4331 216608 52465 16345 22 53 40.1 +44 44 57 5.81 A3Vm+F6V 1.5 0.9 D:AB 5.8 A3VM, 7.8 F6V, 104.5y, a = 0.647", or 102.27y, a = 0.680". Component C, optical.,DYN:0.020".,S:For combined light, Am; K/H/met indicate A3/F0V/F4, respectively.,SB:ADS 16345A.
HR 8712 BD+39 4964 216646 52471 22 54 07.0 +40 22 37 5.81 K0III G:Hyades group.
HR 8718 BD+36 4956 216756 72838 1600 22 55 02.6 +37 04 37 5.91 F5II
HR 8723 BD+35 4917 216831 72851 16376 22 55 44.5 +36 21 06 5.74 B7III 3.7 51.0 S:Hg, Mn.
HR 8725 16 BD+40 4949 216916 52512 16381 EN Lac 22 56 23.6 +41 36 14 5.59 B2IV 3.6 62.1 D:AB relative position of component unchanged in a century. Probably physical. B, 11.5v F0 at 27". C, F5IV, optical, vsini,D:=<54k/s.,G:Lac OB1.,SB:ADS 16381A, 12.097d, K 23.0k/s, V0 -13.0k/s, asini 3.82. RV pulsation 0.169166d.,VAR:ADS 16381A, Beta C, amp. 0.11B, 0.169170, 0.170770 and 0.181692d. Also EA, amp. 0.04V, 12.096816d.
HR 8726 BD+48 3887 216946 52516 I 14368 22 56 26.0 +49 44 01 4.95 K5Ib VAR:Amp. 0.06V.
HR 8731 BD+47 3985 217050 52526 3833 EW Lac 22 57 04.5 +48 41 03 5.43 B4IIIep v RV:Variation in envelope, about 19d. Non-expanding over 50y. Rotating metal shell.,S:Shell star.,VAR:Gamma Cas 5.22 - 5.48V, 5.0 - 5.3p; later observations 5.15 - 5.21V. Amp. variable. Periods at different times have,VAR:varied from 0.7364 in 1951 to between 0.800 and 0.700d; more recent periods were a choice in 1980 between 0.725 and,VAR:0.418d; 0.711 in 1981 and then 0.722d. Also indications of long-term changes. Spectrum variable 2.4 - 10.8y. Spectrum,VAR:also indicates atmospheric quasi-periodic pulsations of about 1d. Strong spectrum and color changes in 1978.
HR 8733 BD+38 4904 217101 72883 3835 22 57 40.7 +39 18 32 6.18 B2IV-V G:Lac OB1.

Legend

Key to columns [154]
HR Harvard Revised Number = Bright Star Number
B Bayer designation (greek letter)
F Flamsteed number
DM Durchmusterung Identification (BD = Bonn; CD = Cordoba; CP = Cape Photographic)
HD Henry Draper Catalog Number
SAO SAO Catalog Number
FK5 FK5 star Number
IR I if infrared source
M* Double or multiple-star code. (A = Astrometric binary; D = Duplicity discovered by occultation; I = Innes, Southern Double Star Catalogue (1927); R = Rossiter, Michigan Publ. 9, 1955; S = Duplicity discovered by speckle interferometry; W = Worley (1978) update of the IDS;)
ADS Aitken's Double Star Catalog (ADS) designation
VarID Variable star identification
RA Right Ascension (J2000.0)
Dec Declination (J2000.0)
vMag Visual magnitude
spType Spectral type
dMag Magnitude difference of double, or brightest multiple
Sep Separation of components in Dmag if occultation binary (arcsec)
Remarks Note on Category (C = Colors; D = Double and multiple stars; DYN = Dynamical parallaxes; G = Group membership; M = Miscellaneous; N = Star names; P = Polarization; R = Stellar radii or diameters; RV = Radial and/or rotational velocities; S = Spectra; SB = Spectroscopic binaries; VAR = Variability)

Quellenangaben