Catalogues

Andromeda / 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 1 BD+44 4550 3 36042 46 00 05 09.9 +45 13 45 6.70 A1Vn 4.2 21.6
HR 8 BD+28 4704 166 73743 69 33 00 06 36.8 +29 01 17 6.13 K0V 2.6 158.6 VAR:6.09 - 6.14V.
HR 15 α 21 BD+28 4 358 73765 1 I 94 Alp And 00 08 23.3 +29 05 26 2.06 B8IVpMnHg v 8.5 81.5 G:Pleiades group.,N:ALPHERATZ; Alpherat; Sirrah; Sirah. Also formerly called Delta Peg.,R:Radius 5 solar.,S:Gallium II lines strong. HgMn star. Spectrum appears earlier at shorter wavelengths.,SB:ADS 94A, 96.6960d, K 30.8k/s, V0 -11.6k/s, asini 34.2.,VAR:Alpha CV 2.02 - 2.06V, 0.9636 or 0.966222d. Some spectral lines vary same period, others half period, some nonvariable.
HR 17 BD+35 8 400 53677 00 08 41.0 +36 37 36 6.19 F8IV
HR 27 22 BD+45 17 571 36123 4 00 10 19.3 +46 04 20 5.03 F2II G:In neutral hydrogen region.
HR 36 BD+47 21 743 36148 I 00 11 59.1 +48 09 09 6.16 gK4
HR 38 BD+36 12 829 53725 00 12 50.4 +37 41 36 6.73 B2V G:Cas-Tau OB1.
HR 40 BD+26 13 895 73823 161 00 13 24.0 +26 59 14 6.30 G0III 1.1 0.1 D:AB 6.7 G3III, 7.5 F2IV, 368y, a = 0.564". ADS 161C, 10.37V, K0, at 18", physical.,DYN:0.0065".,S:Combined spectrum variously classified as F7V, G0V, G0III.
HR 41 23 BD+40 29 905 36173 2010 00 13 30.8 +41 02 07 5.72 F0IV
HR 44 BD+32 21 952 53744 2012 00 14 02.3 +33 12 22 6.25 A1V
HR 52 BD+30 26 1075 53755 I 00 15 07.0 +31 32 09 6.45 R K5
HR 53 BD+26 23 1083 73842 W 00 15 10.6 +27 16 59 6.35 A1Vn 6.8 29.2 SB:Published RV range from -75 to +14k/s.
HR 56 BD+42 41 1185 36221 215 00 16 21.6 +43 35 41 6.15 A2VpSi 3.9 9.2 D:CPM.
HR 63 θ 24 BD+37 34 1280 53777 116 00 17 05.5 +38 40 54 4.61 A2V G:Possible Eggen group with V = +5k/s. Other members: HR 118, 378, 1046, 1706, 2375, 2572, 3131, 3894, 4564, 5482, 5843,,G:6153, 6250, 6355, 6446, 7102, 7124, 7340, 8709.
HR 68 σ 25 BD+35 44 1404 53798 1005 118 00 18 19.7 +36 47 07 4.52 A2V G:Sirius group; UMa stream.,VAR:Delta Sct?, 4.49 - 4.55V.
HR 70 26 BD+42 48 1438 36256 254 119 00 18 42.1 +43 47 28 6.11 B8V 4.1 6.2 D:CPM. Companion F3V.,VAR:ADS 254B, 9.5 - 12v.
HR 71 BD+30 35 1439 53803 1006 00 18 38.3 +31 31 02 5.87 A0IV
HR 75 BD+39 56 1527 36269 00 19 41.6 +40 43 47 6.33 K1III
HR 78 BD+30 42 1606 53820 128 00 20 24.4 +30 56 09 5.90 B7V
HR 79 BD+32 45 1632 53825 I 00 20 45.5 +32 54 41 5.79 K5III
HR 82 ρ 27 BD+37 45 1671 53828 1009 00 21 07.3 +37 58 07 5.18 F5III
HR 90 BD+37 58 1967 53860 I W R And 00 24 02.0 +38 34 38 7.39 S6.5IIIeZr6Ti2 4.9 84.6 S:CO emission. Technetium star, also classified S6.5IIIe, S4/4eZr6Ti2, and S3,5e - S8,8e (M7e).,VAR:M 5.8 - 14.9v, 409.33d.
HR 104 BD+43 92 2421 36390 2027 00 28 13.7 +44 23 40 5.17 A2V s SB:3.9558d, K 41.7k/s, V0 +2.0k/s, asini 2.24.
HR 110 BD+36 66 2507 53928 00 28 56.6 +36 54 00 6.26 G5III
HR 114 28 BD+28 75 2628 74041 409 GN And 00 30 07.3 +29 45 06 5.23 A7III 7.1 139.3 D:ADS 409B 13.3v at 3" CPM with A.,S:Spectrum classified variously as Am, A7III, F0III, F2V.,VAR:Delta Sct 5.18 - 5.22V, 0.0689797d.
HR 122 BD+32 80 2767 53956 W 00 31 25.6 +33 34 54 5.87 K1III 2.4 56.4
HR 128 BD+42 99 2888 36453 00 32 26.8 +43 29 41 6.70 A1Vn S:Also classified A0pSi.
HR 133 BD+26 76 2924 74083 00 32 34.5 +27 34 50 6.67 A2IV
HR 134 BD+27 84 2942 74090 455 00 32 49.1 +28 16 49 6.30 K0III 4.9 8.5 D:ADS 455AB, CPM. B, 10.4v K0V. C, 12.3v at 60".,SB:ADS 455A.
HR 149 BD+26 91 3322 74136 221 00 36 20.0 +27 15 17 6.50 B8IIIpHgMn: SB:Probable SB with period about 400d.,VAR:Amp. 0.06B.
HR 152 BD+43 113 3346 36509 I 00 36 46.6 +44 29 19 5.13 K5-M0III
HR 154 π 29 BD+32 101 3369 54033 18 513 227 00 36 52.9 +33 43 10 4.36 B5V 4.2 35.2 D:AB 103000?y. Component B spectrum A6V or Am(A3/F0/F2), RV +11.9k/s. Component C, 11.4v, F3 at 55" optical.,RV:The secondary has evidently been seen only by J. A. Pearce in 1936.,SB:ADS 513A, 143.6065d, K 47.5k/s, V0 +8.35k/s, msin3i 27.1, asini 77.6. Unresolved by speckle interferometry.
HR 156 BD+23 84 3411 74148 00 37 07.2 +24 00 51 6.47 R K2III
HR 157 BD+34 86 3421 54038 00 37 21.1 +35 23 58 5.48 G2.5IIa
HR 163 ε 30 BD+28 103 3546 74164 19 I 00 38 33.3 +29 18 42 4.37 G6IIIFe-3CH1
HR 165 δ 31 BD+30 91 3627 54058 20 I 548 00 39 19.7 +30 51 39 3.27 K3III 8.2 28.7 D:AB CPM. Component C, 15.2v at 48" optical.,SB:ADS 548A, 15,000d, K 4.0k/s, V0 -8.5k/s, asini 785. Unresolved by speckle interferometry 1983.93.
HR 175 32 BD+38 90 3817 54079 2043 00 41 07.2 +39 27 31 5.33 G8III G:UMa stream.
HR 178 BD+23 94 3883 74200 2044 W 258 00 41 36.0 +24 37 45 6.04 A7m D:Suspected visual double is probably single. Resolved by speckle interferometry 1983.93, sep. 0.145", but unresolved,D:1981.68, 1983.94.
HR 205 BD+44 160 4335 36640 00 46 10.9 +44 51 41 6.05 B9.5IIIpHgMnCr SB:Period at least 2500d.
HR 215 ζ 34 BD+23 106 4502 74267 27 I W Zet And 00 47 20.3 +24 16 02 4.06 K1IIe 5.6 162.7 D:AB CPM. Companions probably optical.,S:CaII emission.,SB:Component A of visual system, 17.7692d, K 26.3k/s, V0 -23.7k/s, asini 6.43. Possible X-ray source 3U0032+24.,VAR:Component A of visual system, EB 3.92 - 4.14V, 17.7695d.
HR 226 ν 35 BD+40 171 4727 36699 1021 00 49 48.8 +41 04 44 4.53 B5V+F8V SB:4.2828d, K 75.6k/s, V0 -23.9k/s, msin3i 1.49, asini 4.45; vsini of secondary 11k/s.
HR 234 BD+44 176 4778 36702 2055 GO And 00 50 18.3 +45 00 08 6.15 A0pCr v S:Possible subdwarf. CrII, MgII, TiII, SrII, EuII but no trace of SiII.,VAR:Alpha CV 6.10 - 6.14V, 2.156d. Also var. K-line, same period.
HR 246 BD+37 159 5066 54225 00 52 53.4 +38 32 55 6.69 A2V
HR 249 BD+36 148 5118 54237 00 53 28.2 +37 25 05 6.06 gK3
HR 258 36 BD+22 146 5286 74359 755 343 00 54 58.0 +23 37 42 5.47 K1IV 0.4 0.6 D:AB 6.02 G6IV, 6.41 K6IV, 164.68y, a = 1.014". Resolved by speckle interferometry 1983.94, sep. 0.68". Combined,D:mag., colors.
HR 269 μ 37 BD+37 175 5448 54281 33 788 00 56 45.2 +38 29 58 3.87 A5V 6.8 266.7 D:All components optical.
HR 271 η 38 BD+22 153 5516 74388 2060 I W 00 57 12.4 +23 25 03 4.42 G8IIIb 6.9 131.7 G:UMa stream.,SB:115.71d, K 17.9k/s, V0 -10.3k/s, msin3i 0.338, asini 28.5; both components vsini <17k/s.
HR 272 BD+45 237 5526 36795 00 57 39.7 +45 50 23 6.12 K2III
HR 275 BD+33 140 5608 54306 2061 00 58 14.2 +33 57 03 5.98 K0
HR 282 BD+43 193 5788 36832 824 B 01 00 03.4 +44 42 40 6.84 H A2Vn 0.8 7.8 D:Visual binary with HR 283.
HR 283 BD+43 193 5789 36833 824 A 01 00 03.6 +44 42 48 6.04 H B9.5Vn 0.8 7.8 D:Visual binary with HR 282. Color for blended images.
HR 289 BD+46 243 6114 36875 862 01 03 01.5 +47 22 34 6.45 A9IV 1.0 0.9 D:6.7 A3n, 8.0, 450y, a = 0.816".,DYN:0.010".,G:Hyades group.,SB:ADS 862A.
HR 290 39 BD+40 209 6116 36874 863 01 02 54.3 +41 20 42 5.98 A5m 6.2 20.9 G:UMa stream.,S:Also classified A3/A7/A9.
HR 305 BD+39 249 6314 54398 01 04 36.4 +39 59 28 6.72 F0Vn
HR 324 41 BD+43 234 6658 36950 2071 01 08 00.9 +43 56 31 5.03 A3m G:Hyades group.
HR 335 φ 42 BD+46 275 6811 36972 940 Var? 01 09 30.2 +47 14 31 4.25 B7Ve 1.2 0.4 D:4.6 B6IV, 5.5 B9V, 371.6y, a = 0.447". Combined mag., colors. Masses 16 and 10 solar. Resolved by speckle,D:interferometry 1983.93, sep. 0.64".,DYN:0.003".,S:Also classified B7III, B9IIIe.
HR 337 β 43 BD+34 198 6860 54471 42 I 949 414 01 09 43.9 +35 37 14 2.06 M0+IIIa e 10.1 80.4 N:MIRACH; Merach; Mirac; Mirak; (al Mizar).,S:Ultraviolet FeII emission. Also classified B9III.
HR 340 44 BD+41 219 6920 36984 2075 01 10 18.8 +42 04 53 5.65 F8V
HR 348 45 BD+36 201 7019 54494 W 01 11 10.3 +37 43 27 5.81 B7III-IV 0.0 0.4 D:Unresolved by speckle interferometry: probably single.
HR 355 BD+44 261 7158 37023 I 01 12 34.0 +45 20 16 6.11 M1III
HR 369 BD+47 357 7546 37067 2085 01 16 24.5 +48 04 56 6.61 B9IIIpSi
HR 372 BD+44 271 7647 37077 I 01 17 05.1 +44 54 07 6.34 R K5
HR 376 BD+46 319 7758 37096 01 18 10.2 +47 25 11 6.25 K0
HR 379 BD+36 220 7853 54592 1055 01 18 47.0 +37 23 10 6.46 A5m 3.1 6.2
HR 390 ξ 46 BD+44 287 8207 37155 1035 I 01 22 20.4 +45 31 44 4.88 K0-IIIb N:Adhil.,SB:17.7673d, asini 6.272.
HR 395 47 BD+36 237 8374 54655 2093 01 23 40.6 +37 42 54 5.58 A2Vm G:Hyades group.,SB:35.371d, K 39.0k/s, V0 +13.3k/s, msin3i 0.440, asini 14.7; vsini same for both components 15k/s.
HR 396 BD+33 220 8375 54654 01 23 37.5 +34 14 45 6.29 G8IV
HR 409 BD+42 302 8671 37204 01 26 18.6 +43 27 28 5.96 F7V
HR 410 BD+33 228 8673 54695 01 26 08.7 +34 34 47 6.31 F7V G:Hyades moving group.
HR 415 BD+33 234 8774 54705 01 27 06.2 +34 22 39 6.27 F7IVb vs G:Hyades moving group.
HR 417 ω 48 BD+44 307 8799 37228 1040 1152 01 27 39.4 +45 24 24 4.83 F5IV 6.6 119.0 D:AB binary, B 11.7v at 2"; CD 10.4, 10.4 sep. 4.9" at 120" from A.,G:Hyades moving group.
HR 418 BD+40 289 8801 37227 1151 01 27 26.6 +41 06 02 6.46 A7m 5.9 15.3 D:Optical.
HR 422 BD+39 334 8837 37234 01 27 47.0 +40 20 08 6.60 A0III G:Member of the local association (Pleiades group); in neutral hydrogen region.,RV:Two published values of vsini are 35 and 135k/s.,S:Shell star.
HR 430 49 BD+46 370 9057 37275 I 01 30 06.2 +47 00 26 5.27 K0III
HR 446 BD+36 277 9531 54788 KK And 01 34 16.6 +37 14 14 5.88 B9IV S:Si star.,VAR:Alpha CV, amp. 0.012V, 0.6684d. Also long-period variations.
HR 452 BD+40 328 9712 37344 01 35 52.5 +41 04 35 6.38 K1III
HR 454 BD+47 460 9746 37351 OP And 01 36 27.2 +48 43 22 5.92 gK1 VARBY, amp. 0.09V. Four minima observed with unequal intervals, about 36 to 66 days superposed on possible secular,VAR:brightening at rate of about 0.045m/100d.
HR 458 υ 50 BD+40 332 9826 37362 1045 I W 01 36 47.8 +41 24 20 4.09 F8V 8.4 114.0 D:Both visual companions probably optical.,SB:197.9d, K 1.8k/s, V0 -27.7k/s, asini 4.79. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,SB:Unresolved by speckle interferometry.
HR 464 51 BD+47 467 9927 37375 52 I 01 37 59.6 +48 37 42 3.57 K3-III N:51 And also called Upsilon Per, but outside IAU boundaries of Perseus.
HR 465 BD+44 341 9996 37393 GY And 01 38 31.7 +45 24 00 6.36 B9pCrEu v S:Spectra show high uranium to thorium ratio. Promethium doubtful. Anomalously high abundance of heavy elements.,S:1000-fold overabundance for the rare earths, Mo and Nb; 100 for Sr and Zr; lanthanides 100,000 times; uranium a million,S:times more abundant than in solar system.,SB:272.99d, K 11.3k/s, V0 -0.55k/s, asini 37.4.,VAR:Alpha CV 6.27 - 6.41V, 36.5d; Sp. and magnetic field var., 22-24y. UII and PmII lines vary in 6.7 hrs.
HR 469 χ 52 BD+43 343 10072 37406 2112 I 01 39 21.0 +44 23 10 4.98 G8III
HR 476 BD+42 345 10204 37419 01 40 39.8 +43 17 52 5.61 sgA9 G:Hyades moving group.
HR 477 τ 53 BD+39 378 10205 37418 1311 584 01 40 34.8 +40 34 37 4.94 B8III 5.9 52.3 D:CPM. Component B, 11.53V, +0.65(B-V), +0.04(U-B).
HR 483 BD+41 328 10307 37434 A 01 41 47.2 +42 36 49 4.95 G1.5V 0.1 D:Astrometric binary 20y, a 0.12", mag. diff 3-4v. Companion 25% solar mass.,G:Hyades group.
HR 495 BD+44 354 10486 37460 01 43 16.5 +45 19 20 6.34 K2IV G:61 Cyg group.
HR 504 BD+45 432 10597 37475 I 01 44 26.5 +46 08 23 6.35 R K5III
HR 518 BD+45 447 10874 37513 2119 01 47 48.0 +46 13 47 6.32 F6V
HR 521 BD+37 372 10975 54991 01 48 38.9 +37 57 10 5.94 K0III
HR 543 55 BD+40 394 11428 37587 2124 I W 01 53 17.3 +40 43 47 5.40 gK1 5.3 59.8
HR 551 BD+39 434 11613 37607 01 54 53.8 +40 42 07 6.24 K2 SB:838d, K 4.30k/s, V0 +31.89k/s, asini 49.6.
HR 552 BD+36 346 11624 55082 I 01 54 57.5 +37 07 42 6.26 K0
HR 556 BD+36 354 11727 55102 I 1534 B 01 55 54.4 +37 16 40 5.89 gM0 0.2 190.4 D:ADS 1534B not CPM with HR 557, component A.,G:Region of NGC 752.
HR 557 56 BD+36 355 11749 55107 1534 A 01 56 09.3 +37 15 06 5.67 K0III 0.2 190.4 D:ADS 1534AP, CPM, 11.9v at 18".,G:Region of NGC 752.
HR 562 BD+40 407 11905 37653 01 57 56.4 +41 41 40 6.78 B8III RV:Hydrogen lines show period 5.01d; metallic lines do not. Possible unseen secondary.,S:HgMn star.
HR 603 γ1 57 BD+41 395 12533 37734 73 I 1630 A 02 03 54.0 +42 19 47 2.26 K3-IIb 2.8 9.6 D:CPM with HR 604.,G:Red star Pleiades group.,N:ALMAAK; Almach; Alamak; Almak; Almaach.
HR 604 γ2 57 BD+41 395 12534 37735 1630 BC 02 03 54.7 +42 19 51 4.84 B8V+A0V 2.8 9.6 D:BC 5.5 B8V, 6.3 A0V, 61.1y, a = 0.296". ADS 1630BC CPM with HR 603. Component D, 15v at 28". Possibly also CPM with,D:BD+41d408 at 53'.,DYN:0.010".,SB:ADS 1630B, 2.67d, K 141k/s, V0 +2.5k/s, msin3i 1.76, asini 4.95; vsini of both components 70k/s.
HR 619 BD+43 431 13013 37794 02 08 33.6 +44 27 34 6.42 R G8III-IV
HR 620 58 BD+37 486 13041 55289 2145 02 08 29.3 +37 51 33 4.82 A5IV-V
HR 628 59 BD+38 425 13294 55330 1683 A 02 10 52.8 +39 02 22 5.63 B9V 0.8 16.2 D:CPM with HR 629.
HR 629 59 BD+38 425 13295 55331 1683 B 02 10 53.7 +39 02 35 6.10 A1Vn 0.8 16.2 D:CPM with HR 628.
HR 643 60 BD+43 447 13520 37867 2153 I S 746 02 13 13.3 +44 13 54 4.83 K3.5IIIBa0.5: SB:748.2d, K4.88k/s, V0 -48.00k/s, asini 47.2.
HR 645 BD+50 481 13530 23047 77 W 747 02 13 36.3 +51 03 57 5.31 G8III: v 4.4 27.3 G:61 Cyg group?,N:6 Per on boundary Per/And.,SB:1650d, K 13.5k/s, V0 +27.3k/s, asini 203. Resolved by speckle interferometry 1981.69, sep. 0.040".
HR 647 BD+46 536 13594 37878 1709 02 14 02.6 +47 29 03 6.06 F4V 0.6 1.0 D:6.6 F3V, 7.08 F6V, 144.7y, a = 0.908". Combined mag., colors.,DYN:0.025".,G:Sirius group; UMa stream.
HR 653 BD+47 590 13818 37905 02 15 57.9 +47 48 41 6.33 R G9III-IV G:Probable Hyades group.
HR 663 BD+43 461a 14028 0 W And 02 17 33.4 +44 18 25 6.70 M7-8Se v M:Proper motion from AGK3. Earlier McCormick determination, +.007",-.002".,S:Also classified S6,1e-S9,2e/M4-M10.,VAR:M 6.7 - 14.6v, 395.93d.
HR 670 62 BD+46 552 14212 37948 1063 02 19 16.8 +47 22 48 5.30 A1V
HR 671 BD+45 589 14213 37947 02 19 10.9 +46 28 21 6.21 A4V
HR 673 BD+48 648 14221 37949 02 19 22.7 +48 57 19 6.37 R F4V
HR 677 BD+39 521 14272 55453 02 19 37.3 +39 50 06 6.63 B8V
HR 679 BD+46 557 14372 37955 02 20 41.4 +47 18 39 6.11 B5V
HR 682 63 BD+49 640 14392 37960 790 02 20 58.2 +50 09 05 5.59 B9pSi VAR:Amp. 0.05U, 1.31d.
HR 687 BD+40 500 14622 37986 2161 W 02 22 50.3 +41 23 47 5.82 F0III-IV 1.8 295.5
HR 694 64 BD+49 649 14770 38005 I 02 24 24.9 +50 00 24 5.19 G8III
HR 699 65 BD+49 656 14872 23319 2165 I W 02 25 37.4 +50 16 43 4.71 K4+III 5.7 191.7
HR 709 66 BD+49 666 15138 23353 02 27 51.8 +50 34 11 6.12 F4V SB:10.9903d, K 46.5k/s, V0 -5.3k/s, msin3i 0.506, asini 6.91.
HR 746 BD+39 573 16004 55680 1961 02 35 27.9 +39 39 52 6.36 B9pHgMn 5.6 16.3 D:Companions optical.
HR 748 BD+36 519 16028 55684 I 1964 02 35 38.8 +37 18 44 5.71 K3III 5.2 18.3
HR 756 BD+38 515 16176 55705 02 36 57.2 +38 43 58 5.90 F5V
HR 760 BD+39 582 16219 55715 02 37 20.8 +39 53 45 6.54 B5V SB:2.089920d, K 21.4k/s, V0 +12.0k/s, asini 0.62.
HR 768 BD+37 588 16327 55729 1996 02 38 17.8 +37 43 36 6.18 F6III 5.0 20.8 D:B 12v, 8" optical; AC CPM; D, mag. diff 5.97v at 40" from A.
HR 769 BD+37 591 16350 55735 02 38 27.8 +38 05 22 6.30 B9.5V S:Also classified A0III.
HR 8744 BD+51 3514 217314 35022 3838 I 22 59 10.3 +52 39 16 6.29 K2
HR 8755 BD+44 4302 217491 52587 23 00 34.4 +45 22 30 6.50 A3V
HR 8758 BD+37 4744 217543 72929 14386 23 00 54.7 +38 42 29 6.54 B3Vpe G:Lac OB1.,S:Shell star.,VAR:Gamma Cas?, 6.53 - 6.60V.
HR 8762 ο 1 BD+41 4664 217675 52609 869 S Omi And 23 01 55.3 +42 19 34 3.62 B6IIIpe+A2p v 0.5 0.3 D:Separate speckle interferometric measures give sep. 0.05" (Aa) and 0.34" (AB). Ten years of observations reveal steady,D:change in AB position angle of about 10d with decrease in separation from about 0.375" to 0.266". Component B,D:identified as SB2 (see SB remarks), making total number of components at least 4.,G:In reflection nebula; probably but not certainly associated.,RV:23.5y. vsini about 300k/s.,S:Shell star. Also classified B5III or B6IVpe.,SB:Speckle interferometry indicates triple star. SB periods 72.3145, 8585 or 9478d. Also short period 1.5845, 0.84,,SB:3.66 or 1.67458d, all doubtful. Observations by Hill et al. (1988, PASP, 100, 243) indicate that one of the companions,SB:of A is SB2, and they identify this as component B. Orbit for B: 33.01d, V0 -14.3k/s, K1 54.8k/s, K2,SB:71.6k/s, m1sin3i 3.74, m2sin3i 2.86, a1sini 0.161, a2sini 0.211.,VAR:Gamma Cas 3.58 - 3.65V. Photometric investigations have indicated numerous periods, particularly 0.78823, 1.0815d and,VAR:1.5998398d, all doubtful. Form of light curve varies. Probably not an eclipsing binary. Period shell phenomena about,VAR:23.5y. Shell features have vanished several times since 1897. H gamma varies in 3.66?d.
HR 8766 2 BD+41 4665 217782 52623 16467 14396 23 02 36.3 +42 45 28 5.10 A3Vn 3.7 0.4 D:AB 5.1 A2, 8.8, 76.6y, a = 0.277".,DYN:0.007".,S:Lambda Boo star.,VAR:ADS 16467B, Delta Sct?, 8.7v.
HR 8768 BD+43 4378 217811 52626 16472 LN And 23 02 45.2 +44 03 32 6.39 B2V 3.9 7.4 D:Fixed. Companion 9.88V, +0.08(B-V), -0.37(U-B), A1V.,G:Lac OB1.,VAR:Amp. 0.02b, 35 min.
HR 8780 3 BD+49 4028 218031 52649 I 23 04 11.0 +50 03 08 4.65 K0IIIbFe-0.5
HR 8800 BD+45 4147 218407 52707 23 07 18.1 +46 04 05 6.66 B2V G:Lac OB1.,SB:3.3378d, K 86.1k/s, V0 -10.3k/s, asini 3.84.
HR 8801 BD+52 3371 218416 35151 23 07 10.1 +52 48 59 6.11 K0III
HR 8804 4 BD+45 4149 218452 52711 3852 I 16526 23 07 39.3 +46 23 14 5.33 K5III 5.5 48.2 G:Sirius group.
HR 8805 5 BD+48 3944 218470 52713 1604 23 07 45.4 +49 17 45 5.70 F5V
HR 8806 BD+43 4399 218525 52717 23 08 12.3 +44 33 42 6.56 A2IV
HR 8825 6 BD+42 4592 218804 52761 3857 23 10 27.2 +43 32 39 5.94 F5IV
HR 8830 7 BD+48 3964 219080 52787 23 12 33.0 +49 24 23 4.52 F0V SB:Unresolved by speckle interferometry 1986.46.
HR 8837 BD+49 4071 219290 35251 23 14 14.3 +50 37 04 6.31 A0V
HR 8857 BD+44 4368 219668 52865 23 17 16.6 +45 09 51 6.43 K0IV
HR 8860 8 BD+48 3991 219734 52871 I 16656 14484 23 17 44.7 +49 00 55 4.85 M2+IIIBa0.3 5.8 219.4 D:AB, CPM. B, 13.0v at 8".
HR 8861 BD+44 4373 219749 52876 ET And 23 17 56.1 +45 29 20 6.48 B9pSi v S:Also classified B8Vp.,SB:48.304d, K 25.7k/s, V0 +2.6k/s, asini 14.8. Possible RV fundamental period 140 min. with 70 and 35 min. harmonics.,VAR:Alpha CV 6.48 - 6.50V, larger amp. in U = 0.05, 0.617135d, 0.49925d. Other periods previously determined range from,VAR:0.44925 to 2.604d. Spectral line strengths vary but not in phase with orbital (SB) period.
HR 8864 9 BD+40 5043 219815 52881 AN And 23 18 23.4 +41 46 25 6.02 A7/8Vm SB:3.219565d, K 71.6k/s, V0 -3.8k/s, asini 3.17. Probable triple system.,VAR:EB 6.0 - 6.16p, A7+A, 3.219565d.
HR 8870 BD+44 4378 219891 52892 23 19 02.4 +45 08 14 6.50 A5Vn
HR 8874 11 BD+47 4110 219945 52907 23 19 29.8 +48 37 31 5.44 K0III
HR 8875 BD+47 4114 219962 52912 W 23 19 41.6 +48 22 51 6.32 K1III 3.3 85.8
HR 8876 10 BD+41 4752 219981 52914 3870 I 23 19 52.4 +42 04 41 5.79 M0III
HR 8884 BD+43 4440 220105 52927 16685 23 20 44.0 +44 06 59 6.13 R A5Vn 4.0 13.2 D:CPM.
HR 8885 12 BD+37 4817 220117 73190 1610 W 23 20 53.3 +38 10 56 5.77 F5V 3.4 121.1
HR 8902 BD+40 5068 220575 52987 23 24 35.0 +41 06 46 6.72 B8III S:Hg, Mn.,SB:212.18d.
HR 8913 13 BD+42 4672 220885 53039 23 27 07.4 +42 54 43 5.75 B9III G:Hyades group.,S:Hg, Mn.
HR 8925 BD+48 4070 221246 53088 3882 I 23 30 07.4 +49 07 59 6.17 K3III G:NGC 7686 #1.
HR 8927 BD+37 4856 221293 73308 23 30 39.7 +38 39 43 6.05 G9III
HR 8930 14 BD+38 5023 221345 73311 I 14599 23 31 17.4 +39 14 11 5.22 K0III
HR 8941 BD+44 4441 221661 53147 23 33 42.7 +45 03 29 6.24 G8II
HR 8947 15 BD+39 5114 221756 73346 1616 14627 23 34 37.5 +40 14 11 5.59 A1Vp G:UMa stream.,S:Lambda Boo star, Mg 4481 wk.
HR 8950 BD+37 4866 221776 73351 I 16843 23 34 46.7 +38 01 26 6.18 K7III 5.2 20.2
HR 8955 BD+32 4671 221970 73368 23 36 30.5 +32 54 15 6.35 F6V
HR 8961 λ 16 BD+45 4283 222107 53204 890 I W Lam And 23 37 33.9 +46 27 29 3.82 G8III-IV v 6.5 217.6 SB:20.5212d, K 6.6k/s, V0 +6.8k/s, asini 1.86. Radio binary. Unresolved by speckle interferometry. Possible radio,SB:emitter.,VAR:RS 3.69 - 3.97V, 4.74 - 5.13B, 54.20d. Amp. and cycle length vary in period 3200d. Also 0.25m var. in period about,VAR:50d. H and K emission correlated with 56d light period.
HR 8962 BD+43 4508 222109 53202 16877 23 37 32.0 +44 25 45 5.80 B8V 0.9 0.5 D:AB 6.3, 7.2v, 351.22y, a = 0.41".
HR 8964 BD+45 4288 222143 53210 23 37 58.6 +46 11 59 6.58 G5
HR 8965 ι 17 BD+42 4720 222173 53216 891 14646 23 38 08.2 +43 16 05 4.29 B8V
HR 8967 18 BD+49 4180 222304 35642 3897 23 39 08.3 +50 28 18 5.30 B9V
HR 8973 BD+36 5098 222399 73422 16913 23 40 02.8 +37 39 09 6.53 F2IV 4.4 14.9 D:CPM.
HR 8976 κ 19 BD+43 4522 222439 53264 1619 16916 23 40 24.5 +44 20 02 4.14 B9IVn 7.6 46.8 D:AB optical.
HR 8977 BD+35 5074 222451 73428 3899 23 40 40.6 +36 43 15 6.23 F1V G:Hyades moving group.
HR 8986 BD+44 4473 222641 53292 I 14674 23 42 14.8 +44 59 31 6.57 R gK5
HR 9003 ψ 20 BD+45 4321 223047 53355 1622 I W 23 46 02.1 +46 25 13 4.95 G5Ib+A0V 4.0 184.0 D:Component A has composite spectrum but star unresolved by interferometer. vsini of G5 component <19:k/s, A0 component,D:=<50k/s. Component B, 14.6v at 25"; C, 13.1v at 62".
HR 9011 BD+46 4169 223229 53374 17006 14709 23 47 33.2 +46 49 57 6.07 B3IV 2.0 0.9 VAR:ADS 17006. Uncertain which component varies.
HR 9024 BD+35 5110 223460 73535 3914 OU And 23 49 41.0 +36 25 31 5.90 G1III e S:CaII emission.,VAR:RS CV, amp. 0.04V, 23.25d.
HR 9053 BD+46 4214 224165 53486 23 55 33.6 +47 21 21 6.00 G8Ib
HR 9057 BD+41 4902 224342 53511 3923 23 57 03.6 +42 39 30 5.97 F8III S:Bidelman classifies gK + F.
HR 9068 BD+31 5012 224544 73650 3927 Var? 23 58 49.2 +32 22 54 6.52 B6IVe S:Shell star.
HR 9070 BD+45 4381 224559 53540 LQ And 23 58 46.5 +46 24 47 6.54 B4Ven v G:Cas-Tau OB1.,S:Shell star. Also classified B3IV.,VAR:Beta C? 6.4 - 6.46B, 0.310049 or 0.622832d. Spectrum variable.
HR 9074 BD+32 4747 224635 73656 17149 A 23 59 29.2 +33 43 28 6.58 H G0V 0.2 1.5 D:AB 6.5 G0V, 6.7 G0V, 355y, a = 3.125". C 12.9V at 82". Blended mag. for HR 9074/5, 5.81V; colors for combined light.
HR 9075 BD+32 4747 224636 73656 17149 B 23 59 29.2 +33 43 28 6.58 H G0V 0.2 1.5 D:Binary with HR 9074, q.v.
HR 9080 BD+44 4538 224801 53568 CG And 00 00 43.7 +45 15 12 6.38 B9pSiEu v S:Enhanced Si, Mn, some rare earths. Magnetic star. Also classified A0Vp.,SB:4.88643d. Other RV periods 3.74d or 2.1 hrs. RV hydrogen lines var. per. about 6 hrs.,VAR:Alpha CV 6.32 - 6.42V, 3.73975d, possible cyclical changes. Also magnetic field and spectrum period. Light var. also,VAR:2.1 hrs. Widths of hydrogen lines in about 35 min. SiII var. in per. 4.88643d.
HR 9086 BD+41 4920 224906 53580 00 01 43.8 +42 22 02 6.25 B9IIIpHg:Mn:
HR 9105 BD+41 4933 225218 36037 I 30 00 04 36.7 +42 05 32 6.01 R B9III 3.7 5.4 D:Binary.,S:Primary discordant classifications, B9III or A3Vs.,SB:ADS 30B, 9.5 F5.
HR 9107 BD+33 4828 225239 53622 2002 00 04 53.8 +34 39 35 6.12 G2V

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)

References