Kataloge

Perseus / 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 470 BD+53 363 10110 22493 I 01 40 13.1 +53 52 06 6.39 K5III
HR 496 φ BD+49 444 10516 22554 57 I Phi Per 01 43 39.6 +50 41 19 4.07 B2Vep G:In neutral hydrogen region; Cas-Tau OB1.,P:Intrinsic polarization, probably due to circumstellar matter.,S:FeII, H in emission. Also classified B0nne, B1III-Vpe.,SB:126.696d. Primary, 16.8k/s, V0 -8.4k/s, msin3i 21.1, asini 29.2; secondary K 105.3k/s, sin3i 3.4,,SB:asini 184. Unresolved by speckle interferometry. Both components appear to be shell stars, B2Ve and B3Ve. Speculation,SB:that secondary is the helium core of a once more massive star whose mass was transferred to the primary.,VAR:Gamma Cas 4.03 - 4.11V, 19.5d. Amp. varies in per. 127d. Possible mass loss. Expanding circumstellar shell.
HR 526 BD+47 508 11031 37536 1438 01 49 15.7 +47 53 49 5.82 A3V 0.7 1.9 D:Component C 8.4v at 21", D 10.2v at 137".,SB:ADS 1438B.
HR 529 BD+51 416 11151 22678 01 50 57.1 +51 56 00 5.90 F5IV
HR 533 1 BD+54 396 11241 22690 2122 V436 Per 01 51 59.3 +55 08 51 5.52 B1.5V G:In neutral hydrogen region; Cas-Tau OB1.,SB:15.6d, K 10k/s, V0 -9k/s.,VAR:E? 5.46 - 5.68y.
HR 536 2 BD+50 379 11291 22696 1052 01 52 09.4 +50 47 34 5.79 B9IIIpHgMn SB:5.6270d, K 26.5k/s, V0 +11.4k/s, asini 2.05.
HR 538 BD+50 381 11335 22705 01 52 50.8 +51 28 29 6.26 A3V
HR 540 BD+54 408 11408 22716 01 53 48.5 +55 35 53 6.45 A5m
HR 568 3 BD+48 576 11949 37665 01 58 33.6 +49 12 15 5.69 K0IV
HR 590 4 BD+53 439 12303 22859 1054 02 02 18.1 +54 29 15 5.04 B8III
HR 618 BD+57 494 12953 22959 V472 Per 02 08 40.5 +58 25 25 5.67 A1Ia t G:NGC 869; Per OB1.,S:Shell star.,VAR:Amp. 0.065V. Sp. var., H alpha profile var.
HR 621 BD+53 460 13137 22993 2146 02 10 07.8 +53 50 35 6.31 G8III
HR 627 5 BD+56 438 13267 23011 1685 Var? 02 11 29.0 +57 38 45 6.36 B5Ia 6.9 60.0 D:B, mag. diff 6.9v at 5.6".,G:Per OB1; h Per.
HR 641 BD+57 519 13476 23044 02 13 41.5 +58 33 40 6.44 A3Iab G:Per OB1; h Per.
HR 654 BD+56 471 13854 23115 W Var? 02 16 51.7 +57 03 19 6.48 B1Iab e 0.9 103.0 G:NGC 869 = h Per; Per OB1.
HR 661 8 BD+57 535 13982 23143 2157 02 17 59.9 +57 53 59 5.75 K3III
HR 662 7 BD+56 486 13994 23149 1753 02 18 04.5 +57 31 00 5.98 G7III 2.6 121.9 C:Heavily reddened.,G:May not be member of Per OB2.,N:Sometimes misidentified as Chi Per.
HR 685 9 BD+55 598 14489 23256 2159 1802 V474 Per 02 22 21.4 +55 50 44 5.17 A2Ia v 7.8 11.6 D:Fixed.,G:Per OB1.,RV:Var. in period over 200d.,S:Shell star.,VAR:Amp. 0.05V. Sp. and H alpha profile var.
HR 690 BD+54 535 14662 23283 1820 V440 Per 02 23 51.8 +55 21 52 6.28 F7Ib 8.1 10.0 VAR:CDelta, amp. 0.123V, 7.572d.
HR 696 10 BD+55 612 14818 23304 Var 02 25 16.0 +56 36 36 6.25 B2Ia e G:Per OB1; in cluster Chi Per; NGC 884.,VAR:Amp. at 0.58 micrometers about 0.15m.
HR 716 BD+54 557 15253 23369 1878 02 29 25.0 +55 32 11 6.51 A2pShell v 1.3 2.8 D:Companion A3IV.,VAR:ADS 1878A, spectrum variable, shell star.
HR 785 11 BD+54 598 16727 23555 2188 02 43 02.8 +55 06 21 5.77 B7IIIpHg SB:Double lines suspected.
HR 787 BD+52 616 16735 23556 2059 02 42 59.7 +53 31 34 5.84 K0II-III 9.0 12.4 D:Optical.
HR 788 12 BD+39 610 16739 55793 2187 S 896 02 42 14.9 +40 11 38 4.91 F9V 0.3 0.1 D:0.906y, a = 0.057".,DYN:0.046".,SB:331.0d, K 21.4k/s, V0 -21.5k/s, msin3i 0.744, asini 72.3. Speckle interferometer measurements combined with,SB:spectroscopic yield masses 1.28 and 1.05 solar. Speckle interferometric sep. 0.047", 1981.68.
HR 792 BD+47 683 16780 38274 2064 02 43 01.9 +48 15 56 6.48 R G5II 5.0 72.8 D:AB fixed.,G:UMa stream.
HR 799 θ 13 BD+48 746 16895 38288 93 I 2081 902 02 44 12.0 +49 13 42 4.12 F8V 5.6 19.6 D:AB 4.13 F7V, 9.87 M1V, 2720y, a = 22.289". C probably optical.,DYN:0.095".
HR 800 14 BD+43 566 16901 38289 1077 02 44 05.2 +44 17 49 5.43 G0Ib-IICa1CH-1
HR 819 BD+35 553 17228 55868 02 46 58.3 +35 59 01 6.25 G8III G:Probable Hyades group.
HR 820 BD+34 513 17240 55872 2117 02 47 03.5 +35 33 18 6.30 R A9V 2.1 1.5 D:AB binary.
HR 825 BD+56 718 17378 23637 S V480 Per 02 49 30.8 +57 05 03 6.25 A5Ia G:Per OB1; vicinity of Perseus double cluster.,VAR:Amp. 0.038V.
HR 831 BD+36 566 17484 55910 02 49 27.1 +37 19 34 6.45 F6III-IV
HR 834 η 15 BD+55 714 17506 23655 99 I 2157 02 50 41.8 +55 53 44 3.76 K3-Ib-IIa e 4.7 28.3 C:Large infrared excess.,D:Component B, B9V, CPM, vsini 149k/s.,G:Red star Pleiades group.,N:Miram in Becvar; Allen says unnamed.,S:Ultraviolet FeII emission. Also classified K3Ib.
HR 840 16 BD+37 646 17584 55928 2194 W 956 02 50 35.1 +38 19 07 4.23 F2III 4.7 249.3 VAR:Delta Sct?
HR 842 BD+46 648 17656 38397 2197 02 51 41.7 +46 50 31 5.88 G8III
HR 843 17 BD+34 527 17709 55946 2198 I A 963 02 51 30.8 +35 03 35 4.53 K5+III S:Also classified K7III.
HR 846 BD+52 640 17743 23674 2185 971 02 52 52.0 +52 59 52 6.36 B8III 0.2 1.6 D:AB, 7.2, 9.2v sep. 0.2" possibly optical; AC binary.,DYN:0.006".
HR 849 BD+47 723 17818 38418 2192 02 53 21.2 +48 34 10 6.26 G5I 5.7 6.7
HR 854 τ 18 BD+52 641 17878 23685 103 I 2202 Tau Per 02 54 15.5 +52 45 45 3.95 G4III+A4V 8.6 51.7 D:A* 4.06 G4III+A4V, 4.150y, a = 0.050". Speckle interferometric sep. 0.080" 1981.67. Circumstellar material surrounding,D:the pair? Visual companions 10.7v at 51" possibly physical; 11.8v at 4" possibly optical.,SB:ADS 2202A, 1515.6d, K 19.0k/s, V0 +2.2k/s, asini 271. vsini of secondary 50k/s.,VAR:EA, 3.94 - 4.07V.
HR 855 20 BD+37 655 17904 55975 2200 977 02 53 42.6 +38 20 15 5.33 F4IV 0.6 0.2 D:AB 5.9 F4V, 6.5 F6V, 31.37y, a = 0.258". Nearly equal components, 3.7, 4.3 solar. Component C, 9.7v at 14", CPM?,DYN:0.013".,SB:ADS 2200A, 1269d, K 4.8k/s, V0 +2.4k/s, asini 73.0. Orbit questioned by Morbey and Griffin (1987, ApJ, 317,,SB:343). Resolved by speckle interferometry 1983.93, sep. 0.20"; 1983.94, sep. 0.18".,VAR:Delta Sct?
HR 864 BD+50 665 18153 23721 02 56 50.6 +51 15 39 6.22 K5III
HR 865 BD+46 658 18155 38455 W 02 56 33.4 +47 09 50 6.02 gK3 5.5 24.9 D:Component B, 15v, possibly spurious.
HR 873 21 BD+31 509 18296 56031 2205 LT Per 02 57 17.3 +31 56 03 5.11 B9pSi v G:Member moving cluster in Perseus.,S:Underabundance of magnesium and oxygen.,SB:2.88d.,VAR:Alpha CV 5.03 - 5.14V, 2.88422d, same for RV and line-intensities. Also var. magnetic field and H-lines. Rotating,VAR:spotted star.
HR 876 BD+38 599 18339 56036 I 02 58 02.3 +38 36 54 6.04 gK3
HR 879 π 22 BD+39 681 18411 56047 2207 02 58 45.7 +39 39 46 4.70 A2Vn N:Gorgonea Secunda.
HR 882 24 BD+34 550 18449 56052 1082 I 02 59 03.7 +35 10 59 4.93 K2III
HR 885 BD+46 669 18474 38493 02 59 49.9 +47 13 15 5.47 G5:III* S:G5:III: CN-4 CH-1 Ca 1 H delta-1. Also classified G8III CH weak. Noted as having composite spectrum, but unresolved,S:by speckle interferometry 1981.69.
HR 886 BD+40 639 18482 38492 I 1004 02 59 39.9 +41 01 59 5.89 K2
HR 890 BD+51 665 18537 23763 2270 A 03 00 52.2 +52 21 06 5.28 B7V 1.4 11.9 D:CPM with HR 891.,G:Per OB3.
HR 891 BD+51 665 18538 23765 2270 B 03 00 53.4 +52 21 08 6.74 B9V 1.4 11.9 D:CPM with HR 890.,G:Per OB1?
HR 894 BD+37 675 18552 56067 03 00 11.8 +38 07 54 6.11 B8Vne S:Shell star. Near IR spectroscopy indicates presence of cool companion.
HR 915 γ 23 BD+52 654 18925 23789 108 I 2324 03 04 47.8 +53 30 23 2.93 G8III+A2V 8.6 57.0 D:SKYLAB observations indicate cool star with hot companion. Components Aa, 14.65y, a = 0.159". Physical nature of B,,D:11m at 57", uncertain.,M:Close to error box of X-ray source 3U0305+53.,SB:5350d, K 12.7 or 21.9k/s, V0 +2.5k/s, msin3i 4.87, asini 648. vsini of secondary 50k/s. Resolved by speckle,SB:interferometry 1981.67, sep. 0.284", 1983.93, sep. 0.27".
HR 918 BD+56 767 18970 23791 2217 I 03 05 32.4 +56 42 21 4.76 G9.5III
HR 920 BD+55 738 18991 23793 03 05 39.9 +56 04 07 6.11 G9III
HR 921 ρ 25 BD+38 630 19058 56138 109 I Rho Per 03 05 10.6 +38 50 25 3.39 M4II G:Zeta Her group.,N:Gorgonea Tertia.,VAR:SRb 3.30 - 4.0V, about 50d with possibly slow var. in mean brightness in 1100d period.
HR 923 BD+40 664 19066 38559 03 05 20.8 +40 34 57 6.05 K0III
HR 930 BD+51 681 19268 23825 03 08 03.9 +52 12 48 6.31 B5V
HR 933 BD+46 692 19279 38587 03 07 47.4 +47 18 30 6.41 A3Vnn
HR 936 β 26 BD+40 673 19356 38592 111 I 2362 Bet Per 03 08 10.1 +40 57 20 2.12 B8V 8.3 81.9 C:Color excess E(B-V) = +0.03.,D:A* var. B8V, 1.858y, a = 0.011" or 1.862y, a = 0.104". Apparent apsidal period 28.4y or 32y. Resolved by speckle,D:interferometry: sep. 0.086", 2-3v fainter than primary. This may be Algol C. Four visual companions all optical:,D:B, 12.7v at 59"; C, 12.5 at 67"; D, 10.5 at 82"; BC sep. 15"; E, 12.5v at 11" from D.,M:One of the few known galactic radio sources in which the dominant star is normal. 21cm radio source.,N:ALGOL; Gorgona; Gorgonea Prima; Demon Star; El Ghoul.,S:B8V+G.,SB:Algol ABxC: 1.8613y, K 12.0k/s, V0 +3.7k/s, msin3i 3.91, asini 109. Spectra B8V, G5IV, Am. Mass Algol AB, 5.3,SB:Suns; C, 1.8 Suns. Circumstellar gas fills Roche lobe of hot component. ADS 19356A: 2.8673d, K 44.0k/s, V0 var.,,SB:asini 1.73. Resolved by speckle interferometry 1982.17, sep. 0.052", 1983.94, sep. 0.08".,VAR:ADS 2362A is the prototype Algol star, first discovered as variable by Montanari in 1669. The first period determined by,VAR:Goodricke in 1783, who also interpreted the variations as due to eclipses. The prototype star proves to be a more,VAR:a complicated system than most of the Algol-type stars, i.e., compact triple system with separation of the components,VAR:well under 0.1". The components usually designated Algol A, B, C, sometimes A, a, P. Two formerly additionally desig-,VAR:nated components D and E, inferred on the basis of an apparent 32 year apsidal motion, are now considered spurious.,VAR:The various Algol components must not be confused with the visual components ADS 2362 B-E, optical companions at much,VAR:greater distances from A. ADS 2362A, EA 2.12 - 3.40V, 2.86732442d, abrupt period changes. Orbital and rotation periods,VAR:synchronized. Rotational velocity 65k/s. Radio flares extending to about 1 A.U., not associated with X-ray activity.,VAR:Radio flare activity appears correlated with period discontinuities, attributed to "starquakes." Mass flow from K to B8,VAR:component at rate of 1.8x10E-08 solar masses/year. Possible circumstellar material associated with radio or H alpha,VAR:emission.
HR 937 ι BD+49 857 19373 38597 112 I W 03 09 04.0 +49 36 48 4.05 G0V 8.2 146.2 G:Mel 20 #44, but not cluster member; Per OB3.
HR 941 κ 27 BD+44 631 19476 38609 I 2368 1055 03 09 29.8 +44 51 26 3.80 K0III 8.4 27.7 D:Companion optical.,G:Hyades group.
HR 947 ω 28 BD+39 724 19656 56224 I W 03 11 17.4 +39 36 42 4.63 K1III 6.1 177.4 N:Gorgonea Quarta.
HR 949 BD+47 779 19735 38638 2225 I W 03 12 26.4 +47 43 33 6.33 K5III 3.9 202.1 G:Mel 20 #138; Per OB3.
HR 950 BD+41 631 19736 38635 03 12 09.6 +42 22 34 6.15 B4V G:Member of the local association (Pleiades group).
HR 956 BD+47 782 19845 38652 03 13 24.0 +48 10 37 5.90 G9III G:Mel 20 #175; Per OB3. Nonmember of Alpha Per cluster on basis of RV.,M:Space motion same as for Hyades cluster.
HR 964 BD+56 798 20041 23903 2424 03 15 48.0 +57 08 27 5.79 A0Ia 8.2 10.8 G:In reflection nebula; member assoc. Cam R1 at about 870 pc. Cam OB1.
HR 966 BD+41 638 20063 38674 03 14 56.7 +42 30 14 6.07 R K2III S:Strong CN.
HR 969 BD+50 729 20123 23914 I 03 16 12.2 +50 56 16 5.03 G6Ib-IIa G:Mel 20 #308; Per OB3.,SB:5.543491d.
HR 973 BD+44 648 20162 38685 I 03 16 04.7 +45 20 45 6.16 M2III
HR 975 BD+32 591 20193 56293 2431 03 15 47.0 +32 51 23 6.31 F4V vw 6.5 44.1
HR 976 BD+34 610 20210 56296 2433 V423 Per 03 16 01.9 +34 41 19 6.25 A1m 7.2 29.3 SB:ADS 2433A, 5.5435d, K 62.7k/s, V0 +24.2k/s, asini 4.78.,VAR:Ell 6.16 - 6.28V, 5.543491d.
HR 978 BD+31 576 20277 56308 03 16 35.1 +32 11 01 6.06 G8IV
HR 979 BD+39 743 20283 38700 2443 03 17 11.4 +40 29 00 6.45 B9VpSi 0.9 3.8 D:Component B, 8.0 A7m. CPM.
HR 982 30 BD+43 674 20315 38704 03 17 47.4 +44 01 30 5.47 B8V G:Per OB3; nonmember of Alpha Per cluster on basis of RV.
HR 986 BD+38 690 20346 56322 2230 03 17 45.8 +39 17 00 5.96 A2IV
HR 987 29 BD+49 899 20365 23944 03 18 37.8 +50 13 20 5.15 B3V G:Per OB3.,SB:1.996933d.
HR 989 31 BD+49 902 20418 38714 03 19 07.6 +50 05 42 5.03 B5V G:Per OB3.
HR 991 BD+33 619 20468 56340 2232 I 03 18 43.8 +34 13 22 4.82 K2IICN1 S:Also classified K2III CN2 Ba 0.3.
HR 1001 BD+48 893 20675 38753 W 03 21 52.6 +49 04 15 5.93 F6V 3.5 205.8 G:Hyades moving group; Per OB3; Mel 20 #497.
HR 1002 32 BD+42 750 20677 38750 2236 1107 03 21 26.5 +43 19 46 4.95 A3V
HR 1011 BD+48 899 20809 38768 03 23 13.2 +49 12 48 5.29 B5V G:Mel 20 #557; Per OB3; nebulosity.,SB:Possibly long period.
HR 1017 α 33 BD+49 917 20902 38787 120 I W 1125 03 24 19.4 +49 51 40 1.79 F5Ib 10.0 167.0 G:Mel 20 #605; Per OB3; nebulosity.,N:MIRPHAK; Mirfak; Marfak; Algenib.
HR 1019 BD+33 636 20995 56419 2514 03 24 29.7 +33 32 09 5.61 R A0V 3.5 4.3 D:AB CPM.
HR 1020 BD+53 657 21004 24024 03 25 48.4 +53 55 18 6.51 A9III-IV
HR 1026 BD+40 736 21038 38809 03 25 09.4 +41 15 26 6.51 A0V
HR 1029 BD+48 913 21071 38817 03 25 57.4 +49 07 15 6.09 B7V G:Mel 20 #675; Per OB3.
HR 1034 BD+48 920 21278 38849 03 28 03.1 +49 03 46 4.98 B5V C:Color excess E(B-V) = +0.10.,G:Mel 20 #774; Per OB3.,S:Lyman alpha observed from COPERNICUS.,SB:21.659d, K 25.0, V0 -0.5, asini 7.34.
HR 1037 BD+49 944 21362 38862 03 28 52.4 +49 50 54 5.58 B6Vn G:Mel 20 #810; Per OB3.
HR 1041 BD+33 656 21402 56475 03 28 20.8 +33 48 27 5.61 R A2V
HR 1044 34 BD+49 945 21428 38872 2558 03 29 22.1 +49 30 32 4.67 B3V 2.1 0.8 D:550y.,G:Mel 20 #835; Per OB3.
HR 1047 BD+46 760 21455 38874 2560 03 29 26.2 +46 56 16 6.24 B7V 5.1 27.9 G:Mel 20 #861; Per OB3. Nonmember of Alpha Per cluster on basis of RV.
HR 1051 BD+47 844 21551 38893 03 30 37.0 +48 06 13 5.82 B8V G:Mel 20 #904; Per OB3.,S:Shell star.
HR 1052 σ 35 BD+47 843 21552 38890 124 I 1167 03 30 34.5 +47 59 43 4.36 K3III G:Mel 20 #900; Per OB3.
HR 1056 BD+48 938 21620 38906 1173 03 31 29.4 +49 12 35 6.29 A0Vn G:Mel 20 #934; Per OB3.,VAR:EA, amp. 0.1V, 5.363d.
HR 1059 BD+48 942 21661 38912 03 31 49.1 +49 24 03 6.39 B9III G:Mel 20 #954; Per OB3.
HR 1063 BD+47 847 21699 38917 V396 Per 03 32 08.6 +48 01 25 5.47 B8IIIpMn G:Mel 20 #985; Per OB3.,S:Spectra show Mn. Helium weak. Si enhanced. Also classified B5Vp.,VAR:Alpha CV 5.45 - 5.53V, 2.4928d. First helium-weak star found to have periodic variations (1973).
HR 1069 36 BD+45 778 21770 38924 2249 1182 03 32 26.3 +46 03 25 5.31 F4III
HR 1072 BD+44 734 21803 38927 KP Per 03 32 39.1 +44 51 20 6.41 B2IV G:Cas-Tau OB1.,VAR:Beta C 6.37 - 6.47V, 0.2101753d, multiple periods, 0.1982, 10.85, 0.01d.
HR 1074 BD+34 674 21856 56531 1098 Var? 03 32 40.0 +35 27 42 5.90 B1V G:Per OB2.
HR 1078 BD+39 811 21912 56538 2254 IW Per 03 33 35.1 +39 53 58 5.81 A5m SB:0.9171877d, K 99.3k/s, V0 +0.2k/s, asini 1.251.,VAR:Ell 5.80 - 5.85V, 0.9171877d.
HR 1087 ψ 37 BD+47 857 22192 38980 I Psi Per 03 36 29.4 +48 11 34 4.23 B5Ve v G:Mel 20 #1164; Per OB3; member of Pleiades group. Nonmember of Alpha Per cluster on basis of RV.,RV:Rotationally unstable shell star.,S:Shell star.,VAR:Amp. 0.04V, 0.5d. Hydrogen emission variable. Expanding circumstellar shell.
HR 1097 BD+42 795 22402 38999 03 38 00.2 +42 34 59 6.42 B8Vn
HR 1113 BD+37 811 22780 56628 1225 03 41 07.9 +37 34 48 5.57 B7Vne G:Member of the local association (Pleiades group).,VAR:Gamma Cas?, 5.55 - 5.58V.
HR 1122 δ 39 BD+47 876 22928 39053 131 W Del Per 03 42 55.5 +47 47 15 3.01 B5IIIe t 7.3 99.1 C:Color excess E(B-V) = +0.04.,G:Per OB3.,S:C1 neutral carbon continuum shows discontinuities in UV. Lyman alpha observed from COPERNICUS.,VAR:Alpha CV? 2.98 - 3.03V, about 1d. Strong variable emission at 1650A, CaII?
HR 1123 40 BD+33 698 22951 56646 2699 03 42 22.5 +33 57 54 4.97 B0.5V 5.0 20.0 C:Reddened star. Color excess E(B-V) = +0.24.,G:Per OB2.
HR 1127 BD+48 984 23049 39063 I 2712 03 44 06.4 +48 31 25 6.06 K4III 7.1 18.6 C:Nicolet has 6.60V, Mermilliod 6.39V: no indication of variability.
HR 1130 BD+45 804 23139 39071 2266 03 44 40.9 +46 05 59 6.11 A7IV
HR 1131 ο 38 BD+31 642 23180 56673 2726 Omi Per 03 44 19.1 +32 17 18 3.83 B1III 2.8 1.0 C:Reddened star. Color excess E(B-V) = +0.32.,D:Binary. Combined mag., colors. Rotational velocity B, 150:k/s. Unresolved by speckle interferometry 1982.16.,DYN:0.005".,G:Per OB2 (not a member). Embedded in reflection nebulosity. In cluster IC 348.,M:In interstellar ultraviolet radiation field.,N:Atik; Ati; Al Atik.,P:Intrinsic polarization, probably due to circumstellar matter.,SB:4.4192d, K 109.3k/s, V0 +19.8k/s, msin3i 5.26, asini 6.63. Rotational velocity of secondary, 84k/s, primary,SB:85k/s.,VAR:Ell 3.79 - 3.85V, 4.419171d, possibly half.
HR 1133 BD+36 742 23193 56675 2268 03 44 31.4 +36 27 36 5.59 A2m
HR 1135 ν 41 BD+42 815 23230 39078 134 I 2738 1261 03 45 11.6 +42 34 43 3.77 F5II 8.1 31.4
HR 1141 BD+45 811 23300 39085 2746 03 45 59.3 +45 40 55 5.66 B6V 8.4 6.5 D:CPM.,G:Member of the local association (Pleiades group).
HR 1160 BD+50 825 23552 24231 2769 03 48 18.3 +50 44 12 6.14 B8Vne 6.2 7.0 D:Probably optical.,S:Shell star.
HR 1163 BD+33 717 23625 56709 2772 1305 03 47 52.6 +33 36 00 6.57 B2.5V 4.0 3.2 D:Binary.,G:Per OB2.,SB:ADS 2772A, 1.9406d, K 82k/s, V0 +20k/s, msin3i 0.883, asini 2.19.,VAR:B-A varies from 2.8 to 4.3V. Uncertain which component varies.
HR 1164 BD+31 650 23626 56707 03 47 48.9 +32 11 42 6.25 G0
HR 1170 BD+43 818 23728 39128 V376 Per 03 49 08.2 +43 57 47 6.02 A9IV VAR:Delta Sct 5.8 - 5.91V, variable amp. Primary and beat periods, 0.098299 and 0.39206d.
HR 1176 BD+44 801 23838 39134 Var? 03 50 04.5 +44 58 04 5.66 G2III+F2:V SB:vsini of secondary 85k/s. Unresolved by speckle interferometry 1983.93.,VAR:A variable comparison star was used when HR 1176 was suspected of variablility.
HR 1177 42 BD+32 667 23848 56727 V467 Per 03 49 32.6 +33 05 29 5.11 A3V G:Per OB2.,SB:1.7653d, K 34.4k/s, V0 -11.9k/s, asini 0.832.,VAR:A published period, 22.58d, does not satisfy available SB observations, whereas the SB period does satisfy the,VAR:photometric equally well. However, more observations are badly needed.
HR 1191 BD+33 728 24131 56761 W 03 51 53.7 +34 21 33 5.77 B1V 7.5 15.1 G:Per OB2.
HR 1197 BD+30 582 24167 56762 03 52 04.3 +31 10 06 6.25 A5V G:Per OB2.
HR 1198 BD+48 1015 24240 39175 03 53 38.7 +48 39 02 5.76 K0III
HR 1203 ζ 44 BD+31 666 24398 56799 144 I 2843 1397 03 54 07.9 +31 53 01 2.85 B1Ib 6.5 12.9 C:Reddened star. Color excess E(B-V) = +0.33.,D:AB CPM, B 9.16V B8IV; C, 9.12V at 33" optical; D, 10.35V, +0.713(B-V), +0.20(U-B), at 92" optical; E, 9.90V, A2V,,D:+0.33(B-V), +0.17(U-B), at 120" physical.,DYN:0.012".,G:IC 348; Per OB2.,RV:Comp. B +20.8k/s.,S:Interstellar CH detected optically. COPERNICUS data used to analyze the chemical abundances in line of sight to,S:Zeta Per: CO, HD, and OH. About 60% of the hydrogen in front of the star is molecular.,SB:1.765d, K 6.0k/s, V0 +22.2k/s.,VAR:2.80 - 2.93V.
HR 1207 BD+47 912 24504 39195 2279 03 55 58.2 +47 52 17 5.37 B6V G:Per OB3.
HR 1209 BD+30 591 24534 56815 I 2859 X Per 03 55 23.0 +31 02 45 6.10 O9.5ep v 5.8 22.5 C:Heavily reddened.,D:CPM? Component A possibly optical counterpart or companion of X-ray source 4U0352+30. Possibly a triple system with a,D:neutron star moving around the optical primary in 22.4 hrs., and either apsidal period 581d or close double moving,D:around a distant component in 581d. Rotational velocity of primary, vsini 306k/s. Component ADS 2859B is normal M1III,,D:not T Tau type as once assumed.,G:May not be member of Per OB2; Zeta Per group.,M:Space velocities of X Per and Xi Per indicate the two stars approached to within 17 pc 2 million yrs ago.,P:Conflicting evidence whether observed polarization is intrinsic to the star or of interstellar origin.,S:Sp. data suggest occasional interruption of almost steady infall of material through rotating emission region by,S:outbursts of material from the star.,SB:580.7d, K 59k/s, V0 -50k/s, asini 471. Emission lines var. in RV, 22.4 hrs. and 581d.,VAR:ADS 2859A, Gamma Cas 6.07 - 7.0V, 580.7?d. Amp. about 0.02U. X-ray period 22.4 hrs. Spectrum variable. Sudden,VAR:decrease in H alpha emission followed by 450 sec. flare in continuum. Possible neutron star companion pulsating in,VAR:13.924 min. Simultaneous X-ray and optical obs. 21 Jan. 1975 showed X-ray var. by factor 2 but no corresponding optical,VAR:100 sec. quasi periodic photometric var. may indicate binary with compact companion undergoing mass accretion.
HR 1210 43 BD+50 860 24546 24314 I W 03 56 36.5 +50 41 43 5.28 F5IV 4.8 75.3 C:IR source in this direction corresponds to a Seyfert galaxy.,D:AB CPM. Component C, 11.4v at 101" optical. P, 12.5v at 279".,G:Hyades moving group.,SB:30.4380d, K 51.9k/s, V0 +25.1k/s, msin3i 0.910, asini 16.9; alternate orbit 30.4391d, K50.6k/s,,SB:msin3i 0.82, asini 15.53; vsini both components <17k/s.
HR 1215 BD+34 768 24640 56824 1418 03 56 28.7 +35 04 52 5.49 B1.5V G:Per OB2.,VAR:Beta C?, 5.45 - 5.50V. RV possibly var. 0.13169d.
HR 1220 ε 45 BD+39 895 24760 56840 147 2888 Eps Per 03 57 51.2 +40 00 37 2.89 B0.5V+A2V 5.1 8.8 C:Color excess E(B-V) = +0.10.,D:AB CPM. B, 7.39V, -0.03(B-V), -0.52(U-B), B9.5V, vsini 300:k/s.,G:Cas-Tau OB1; member of Pleiades group.,VAR:Beta C, 2.88 - 3.00V, 0.216:d. Brightest component on visual triple. Photoelectric and spectroscopic resonant periods,VAR:found are submultiples of 26.9 hrs or 1.12d.
HR 1223 BD+34 773 24809 56847 V386 Per 03 58 03.1 +34 48 52 6.53 A8V G:Per OB2.,SB:vsini both components 80k/s.,VAR:Delta Sct 6.50 - 6.58V, 0.052d.
HR 1226 BD+38 827 24843 56849 03 58 29.1 +38 50 25 6.30 gK1
HR 1228 ξ 46 BD+35 775 24912 56856 148 I Xi Per 03 58 57.9 +35 47 28 4.04 O7.5III(n)((f)) e C:Color excess E(B-V) = +0.32.,G:Runaway star from Per OB2. Within 1d and exciting star of HII region S220. Ionizes region at edge of California nebula =,G:NGC 1499.,N:Menkib; Menkhib; Menchib.,S:Interstellar CO emission. Central Balmer emission in blue-violet only.,SB:6.951d.,VAR:Slightly variable, possibly same period as SB.
HR 1229 BD+38 829 24982 56866 2910 03 59 40.0 +38 49 14 6.38 R A1Vp: 2.7 1.5
HR 1234 BD+36 805 25152 56899 04 01 14.7 +36 59 24 6.41 A0V RV:Determinations of vsini range from 50 to 250k/s.
HR 1261 λ 47 BD+49 1101 25642 24412 1113 04 06 35.0 +50 21 05 4.29 A0IVn
HR 1273 48 BD+47 939 25940 39336 152 I MX Per 04 08 39.7 +47 42 45 4.04 B3Ve G:Per OB3; member of Pleiades group.,RV:Pole on.,S:Excess IR emission.,SB:16.934615d not confirmed.,VAR:Gamma Cas 4.00 - 4.10V, 55?d. Slow var. possibly associated with emission spectrum.
HR 1277 49 BD+37 881 25975 57000 04 08 15.3 +37 43 40 6.09 K1III
HR 1278 50 BD+37 882 25998 57006 2297 04 08 36.6 +38 02 23 5.51 F7V D:CPM with GC 4949 at 12' = ADS 2995, a triple system 7.3 dK2, 9.0 sep. 1"; C at 234".,G:Hyades group.
HR 1286 BD+33 807 26311 57047 2300 I 04 10 59.0 +33 35 12 5.72 K1II-III
HR 1301 BD+37 897 26605 57081 04 13 59.6 +37 58 01 6.45 R G9III
HR 1303 μ 51 BD+48 1063 26630 39404 1117 I 3071 1518 04 14 53.9 +48 24 34 4.14 G0Ib 6.0 83.8 D:A* 4.13 G0Ib, 0.778y, a = 0.019". AB CPM; B, 11.8v at 15". C , 10.25V, +0.47(B-V), +0.06(U-B), B8.,SB:283.272d, K 20.7k/s, V0 +7.7k/s, asini 80.5. Unresolved by speckle interferometry.,VAR:ADS 3071A, 4.1 - 4.24V.
HR 1306 52 BD+40 912 26673 39409 2306 I 04 14 53.3 +40 29 01 4.71 G5Ib+A2V SB:1576.44d, K 18.1k/s, V0 -4.5k/s, asini 358. Unresolved by speckle interferometry 1983.93. vsini of secondary,SB:100k/s.
HR 1324 BD+49 1150 26961 24531 b Per 04 18 14.6 +50 17 44 4.61 A2V G:In NGC 1545 #1; Hyades group.,M:Source of weak radio emission.,SB:Comp. ABC: 701.76d, K 11.4k/s, V0 +21k/s, asini 107. Comp. A: 1.527365d, K 39.4k/s, V0 var., asini 0.827.,SB:Unresolved by speckle interferometry.,VAR:Ell 4.59 - 4.65V, 1.527365d. Radio binary showing radio flare activity. Third component may eclipse primary.
HR 1328 BD+41 844 27026 39447 04 18 08.2 +42 08 28 6.22 B9V
HR 1330 BD+49 1155 27084 39457 04 19 13.3 +50 02 56 5.45 A7V G:NGC 1545 #1.
HR 1333 BD+50 973 27192 24544 2316 1550 04 20 11.5 +50 55 15 5.55 B1.5IV G:Cas-Tau OB1.,SB:1.527365d, K 38.83k/s, V0 +20.66k/s, asini 0.815.,VAR:Amp. 0.020V.
HR 1337 BD+41 852 27278 39468 04 20 14.4 +41 48 29 5.92 K0III
HR 1343 54 BD+34 860 27348 57171 158 I W 04 20 24.6 +34 34 00 4.93 G8III 7.9 110.0
HR 1344 BD+31 757 27349 57166 I 04 20 10.0 +31 57 12 6.16 K5
HR 1350 53 BD+46 872 27396 39483 2319 V469 Per 04 21 33.2 +46 29 56 4.85 B4IV G:Member of Pleiades group.,SB:Same period as VAR.,VAR:Amp. 0.01V, 7.29?hrs.
HR 1371 BD+42 946 27650 39501 3172 04 23 35.9 +42 25 41 6.23 A1pSi 0.5 0.4
HR 1377 55 BD+33 853 27777 57212 04 24 29.2 +34 07 50 5.73 B8V
HR 1379 56 BD+33 854 27786 57216 3188 1592 04 24 37.4 +33 57 35 5.76 F4V 3.6 4.9 DYN:0.042".,VAR:ADS 3188B, 9.6 - 11.3v.
HR 1390 BD+31 776 27971 57229 2325 04 26 06.3 +31 26 20 5.28 K1III
HR 1419 BD+32 806 28459 57269 W 04 30 38.3 +32 27 29 6.21 B9.5Vn D:Suspected of being double; probably single.
HR 1424 BD+39 1013 28503 57278 3273 A 04 31 24.0 +40 00 37 6.26 B8V 0.5 9.3 D:CPM.
HR 1434 57 BD+42 990 28704 39604 1124 W 04 33 24.9 +43 03 50 6.09 F0V 0.7 116.2
HR 1454 58 BD+40 1000 29094 39639 2338 I A 04 36 41.4 +41 15 53 4.25 K4III+A3V 0.1 D:A* 4.27 G8II+B, 28.67y, a = 0.054"(not confirmed).,S:Also classified K0II-III + B9V.,SB:10,470d, K 12.8k/s, V0 +5.9k/s, asini 1400. One of the longest SB periods known, 28.67y. Masses 6 and 5 solar.,SB:Unresolved by speckle interferometry. vsini of both components =<50k/s.
HR 1482 BD+48 1128 29526 39688 2347 04 41 24.1 +48 18 03 5.67 A0V
HR 1489 BD+37 954 29645 57377 2348 04 41 50.3 +38 16 49 5.99 G0V
HR 1493 BD+49 1230 29721 39702 1128 W 04 43 21.6 +49 58 26 5.87 B9III 7.3 20.8
HR 1494 59 BD+43 1043 29722 39699 2349 04 42 54.3 +43 21 54 5.29 A1Vn
HR 1500 BD+40 1032 29866 39715 04 44 12.9 +40 47 13 6.08 B8IVne S:Shell star.
HR 1514 BD+40 1045 30138 39746 04 46 44.4 +40 18 46 5.97 G9III
HR 1533 BD+37 969 30504 57447 1133 I 04 49 54.6 +37 29 18 4.88 K3.5IIIBa0.2: N:Formerly 1 Aur, now in Perseus.

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)

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