Catalogues

Serpens / 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 5654 BD+19 2935 134943 101429 3199 I W FL Ser 15 12 04.3 +18 58 33 5.89 M4IIIab 1.9 0.5 D:Resolved by speckle interferometry 1986.45, sep. 0.51".,VAR:Lb 5.79 - 6.02V.
HR 5659 BD+19 2939 135101 101437 9535 A 15 12 43.5 +19 17 09 6.68 G5V 0.8 23.7 D:Binary. Companion 7.53V, +0.35(R-I), dG6.,DYN:0.038".,G:Epsilon Ind group.
HR 5665 BD+23 2789 135263 83723 3201 15 13 31.9 +22 59 00 6.30 A2V
HR 5675 3 BD+05 2985 135482 120916 562 I 15 15 11.4 +04 56 22 5.33 K0III
HR 5679 4 BD+00 3327 135559 120920 15 15 49.1 +00 22 20 5.63 A4V
HR 5690 BD+00 3337 136028 140444 I 15 18 26.2 -00 27 41 5.89 K5III
HR 5692 BD+21 2755 136138 83755 1400 15 18 24.5 +20 34 22 5.70 G8IIIaBa0.3
HR 5694 5 BD+02 2944 136202 120946 9584 MQ Ser 15 19 18.8 +01 45 55 5.06 F8III-IV 4.6 11.2 D:AB binary. Some disagreement as to whether B or C, at 127" from A, is the brighter.,DYN:0.034".,G:Not member of Gamma Leo group but previously listed as such.
HR 5706 BD-01 3047 136442 140473 15 20 47.1 -02 24 48 6.35 K0V
HR 5710 6 BD+01 3067 136514 120955 I 9596 7037 15 21 02.0 +00 42 55 5.35 K3III 4.0 3.1 D:CPM?,DYN:0.013".,G:Wolf 630 group.
HR 5711 BD+25 2902 136643 83778 15 21 06.9 +24 57 28 6.39 K0
HR 5717 7 BD+13 2928 136831 101508 3213 15 22 23.2 +12 34 03 6.28 A0V
HR 5721 8 BD-00 2961 137006 140502 1406 15 23 43.7 -01 01 21 6.12 F0V G:UMa stream.
HR 5739 τ1 9 BD+15 2858 137471 101545 570 I 7074 15 25 47.4 +15 25 41 5.17 M1III
HR 5740 BD+19 2966 137510 101548 15 25 53.3 +19 28 51 6.27 G0IV-V M:Possible nearby star on basis of spectroscopic parallax.
HR 5745 BD+25 2916 137853 83830 3219 I 15 27 38.9 +25 06 06 6.02 gM1
HR 5746 10 BD+02 2965 137898 121020 3221 15 28 38.2 +01 50 32 5.17 A8IV
HR 5758 BD+09 3055 138290 121038 1408 15 30 55.4 +08 34 45 6.57 F4V w
HR 5770 τ2 12 BD+16 2797 138527 101600 15 32 09.7 +16 03 22 6.22 B9V
HR 5772 11 BD-00 2982 138562 140596 3226 15 32 57.9 -01 11 11 5.51 K0III
HR 5783 BD+17 2880 138803 101618 15 33 52.8 +17 08 16 6.45 R F3III
HR 5788 δ 13 BD+11 2821 138917 101623 9701 B 15 34 48.1 +10 32 15 3.80 F0IV 1.1 3.9 D:ADS 9701, 3168y, a = 5.8432". Binary with HR 5789, blended mag., colors.,DYN:0.022".
HR 5789 δ 13 BD+11 2821 138918 101624 9701 A Del Ser 15 34 48.1 +10 32 21 3.80 F0IV 1.1 3.9 D:Binary with HR 5788. CD 13.5, 14.0 sep. 4" at 65" from A, optical.,DYN:0.022".,VAR:Delta Sct 4.20 - 4.25V, 0.134d. Fourier analysis of 1975 and 1979 data shows frequencies of 6.4227 and 7.8869 cycles/d,VAR:or periods 0.1557 and 0.1268d.
HR 5791 BD+02 2977 138936 121071 15 35 04.6 +01 40 08 6.56 F0III
HR 5795 τ3 15 BD+18 3044 139074 101631 3230 15 35 33.2 +17 39 20 6.12 gG8
HR 5796 BD+11 2826 139087 101634 3231 15 35 53.4 +11 15 56 6.07 gK0
HR 5799 14 BD-00 2988 139137 140643 15 36 33.7 -00 33 42 6.51 G8III+A
HR 5802 16 BD+10 2884 139195 101640 15 36 29.6 +10 00 36 5.26 K0III:CN1Ba0.7Sr2
HR 5804 τ5 18 BD+16 2807 139225 101642 15 36 29.3 +16 07 08 5.93 F3V S:Also classified F0IVn.
HR 5831 BD+12 2875 139862 101673 9740 15 40 10.4 +12 03 11 6.25 G7.5IIIaFe-0.5 4.2 16.5 D:Companion 10.33V, +0.49(B-V), -0.01(U-B), F5V, CPM.,S:G8.5IIIa CN-1 Ca-1 Fe 0.5.
HR 5840 τ6 19 BD+16 2816 140027 101678 15 40 59.2 +16 01 29 6.01 G8III G:Sirius group; UMa stream.
HR 5842 ι 21 BD+20 3138 140159 101682 9744 15 41 33.1 +19 40 13 4.52 A1V 0.1 0.1 D:AB 5.2 A1V, 5.3 AIV, 11.07y, a = 0.117". AB combined mag., color. Resolved by speckle interferometry 1986.45,,D:sep. 0.05".,DYN:0.012" to 0.026".,G:Pleiades group.
HR 5843 χ 20 BD+13 2982 140160 101683 3243 Chi Ser 15 41 47.4 +12 50 51 5.33 A0pSr v G:In Ursa cluster; UMa stream. Possible Eggen group with HR 63, q.v.,VAR:Alpha CV 5.33 - 5.36V, 1.59584d. SrII same period. Magnetic field var. Period probably due to rotation of star,VAR:spots.
HR 5845 τ7 22 BD+18 3059 140232 101686 15 41 54.7 +18 27 50 5.81 A2m G:Hyades group.,S:Also classified A8Vams.
HR 5850 BD+14 2922 140438 101699 9758 15 43 10.6 +13 40 04 6.48 G5III 1.0 0.6
HR 5853 ψ 23 BD+02 2989 140538 121152 3248 9763 15 44 01.8 +02 30 54 5.88 G2.5V 1.3 370. D:Quintuple system of which E is brightest companion; B, 12.0V at 4"; others at 172" and 208".,DYN:0.084".
HR 5854 α 24 BD+06 3088 140573 121157 582 I 9765 15 44 16.1 +06 25 32 2.65 K2IIIbCN1 8.3 58.2 D:SR? Amp. 0.2V. ADS 9765B, optical.,N:UNUKALHAI; Unuk al Hay; Unuk Elhaia; Unuk; Unukalhay; Cor Serpentis.
HR 5858 τ8 26 BD+17 2906 140729 101712 S 15 44 42.1 +17 15 51 6.14 A0V 0.1
HR 5859 BD+05 3072 140775 121170 15 45 23.5 +05 26 49 5.58 A0V G:UMa stream.
HR 5861 BD+01 3125 140815 121173 15 45 39.7 +00 53 29 6.33 K0III
HR 5863 25 BD-01 3092 140873 140740 15 46 05.6 -01 48 16 5.40 B8III SB:38.937d, K 53.6k/s, V0 -12.6k/s, asini 17.2. Unresolved by speckle interferometry.
HR 5867 β 28 BD+15 2911 141003 101725 583 9778 15 46 11.3 +15 25 19 3.67 A2IV 6.3 30.6 D:B, 9.72V, +0.84(B-V), +0.68(U-B), K3V, CPM. C, 10.7v at 201". Also CPM with BD+15d2906 at 1642", itself a double, 8.4,,D:10.5v sep. 6".,DYN:0.016".,G:Sirius group; member of Ursa cluster; UMa stream.,RV:ADS 9778B, +2.8k/s.
HR 5868 λ 27 BD+07 3023 141004 121186 I 7246 15 46 26.6 +07 21 11 4.43 G0-V SB:1837d, K 2.8k/s, V0 -6.7k/s, asini 59.1. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).
HR 5870 υ 31 BD+14 2939 141187 101739 15 47 17.3 +14 06 55 5.71 A3V G:Hyades group.
HR 5874 BD+14 2940 141353 101744 I 15 48 13.3 +13 47 19 6.00 gK2
HR 5879 κ 35 BD+18 3074 141477 101752 584 I 7269 15 48 44.4 +18 08 30 4.09 M0.5IIIab e S:Ultraviolet FeII emission.
HR 5881 μ 32 BD-02 4052 141513 140787 585 15 49 37.2 -03 25 49 3.53 A0V
HR 5888 ω 34 BD+02 3007 141680 121215 I 15 50 17.5 +02 11 47 5.23 G8III G:UMa stream.,S:Also classified A6IVm.
HR 5892 ε 37 BD+04 3069 141795 121218 588 15 50 49.0 +04 28 40 3.71 A2Vm S:Also classified A6IVm.
HR 5894 BD+15 2918 141850 101771 I R Ser 15 50 41.7 +15 08 01 5.20 M7IIIe VAR:M 5.16 - 14.4v, 356.41d.
HR 5895 36 BD-02 4058 141851 140801 S 15 51 15.6 -03 05 26 5.11 A3Vnp 0.1 S:Lambda Boo star, Mg 4481 wk.
HR 5899 ρ 38 BD+21 2829 141992 84037 I 7300 15 51 15.9 +20 58 40 4.76 K5-III
HR 5909 BD+17 2926 142244 101789 15 52 56.2 +17 24 13 6.36 R K0
HR 5911 39 BD+13 3024 142267 101792 3254 W 7313 15 53 12.1 +13 11 48 6.10 G0VFe-0.5 5.6 98.3
HR 5913 BD+16 2840 142357 101796 9828 15 53 34.9 +16 04 30 6.09 R F5II-III 6.4 3.6 S:Also classified F4IVs or F3V.
HR 5919 40 BD+09 3116 142500 121254 3256 FP Ser 15 54 40.3 +08 34 49 6.29 A7Vn VAR:Delta Sct 6.20 - 6.23V, about 0.250d.
HR 5924 BD+20 3166 142574 84070 3257 I 15 54 34.6 +20 18 39 5.44 M0III G:Epsilon Ind group.,M:High space velocity.
HR 5931 BD+19 3036 142763 101821 15 55 39.8 +18 37 14 6.26 B8III M:Old disk population runaway star.
HR 5933 γ 41 BD+16 2849 142860 101826 591 I W 7350 15 56 27.2 +15 39 42 3.85 F6V 6.6 201.5 C:Color excess E(B-V) = +0.03.,D:Companions optical?
HR 5940 φ BD+14 2969 142980 101834 I 15 57 14.6 +14 24 52 5.54 K1IV
HR 5963 BD+04 3096 143553 121315 3262 16 00 51.1 +04 25 39 5.83 gK0
HR 5972 π 44 BD+23 2886 143894 84155 3268 16 02 17.7 +22 48 16 4.83 A3V
HR 5976 43 BD+05 3131 144046 121339 W 16 03 45.7 +04 59 12 6.08 G9III 7.8 30.8 G:Probable Hyades group.
HR 5992 BD+08 3134 144426 121361 16 05 37.8 +08 05 46 6.29 A3m SB:8.855d, K 31.6k/s, V0 -21.5k/s, asini 3.56.
HR 6004 45 BD+10 2958 144874 101939 3274 16 07 37.5 +09 53 30 5.63 A7V
HR 6005 BD+22 2926 144889 84202 I 16 07 22.2 +21 49 21 6.14 K4III
HR 6010 47 BD+08 3141 145002 121383 I FS Ser 16 08 28.0 +08 32 03 5.73 M3.5IIIa VAR:Amp. 0.04V.
HR 6011 BD+03 3132 145085 121390 I 16 08 58.9 +03 27 16 5.91 gK5
HR 6014 BD+06 3169 145148 121392 1422 16 09 11.2 +06 22 44 5.97 K1.5IV
HR 6016 BD-03 3884 145206 141001 I 16 09 50.5 -03 28 01 5.37 K4III SB:Companion may be the cause of bright UV in spectrum.
HR 6093 σ 50 BD+01 3215 147449 121540 1427 16 22 04.4 +01 01 45 4.82 F0V G:Hyades group.
HR 6446 ν 53 BD-12 4722 156928 160479 3376 10481 17 20 49.7 -12 50 49 4.33 A2V 4.8 46.3 G:Possible Eggen group with HR 63, q.v.
HR 6449 BD-10 4477 156971 160482 W 17 20 52.7 -10 41 46 6.46 F1III 7.8 8.1
HR 6496 BD-12 4750 157968 160553 17 27 02.1 -12 30 45 6.21 F7V N:Originally called 47 Oph; now in Serpens.
HR 6544 BD-11 4411 159358 160653 1461 W 17 34 46.4 -11 14 31 5.55 B8Vn 3.0 54.6 G:Sco-Cen assoc.
HR 6561 ξ 55 BD-15 4621 159876 160700 658 I W 9270 17 37 35.2 -15 23 55 3.54 F0IVDel Sct 9.4 22.0 D:Visual companion optical.,G:Hyades moving group.,SB:2.2923d, K 19.4k/s, V0 -42.8k/s, asini 0.612.,VAR:Delta Sct?, 3.52 - 3.54V.
HR 6562 BD-15 4622 159877 160701 17 37 36.2 -15 34 16 5.94 F0IV
HR 6568 BD-10 4528 160018 160708 I 17 38 09.5 -10 55 35 5.75 gK0
HR 6581 ο 56 BD-12 4808 160613 160747 3405 Omi Ser 17 41 24.9 -12 52 31 4.26 A2V VAR:Delta Sct 4.20 - 4.26V, 0.053d.
HR 6600 BD-13 4732 161023 160784 17 43 48.6 -13 30 31 6.39 F0V
HR 6620 BD-14 4770 161701 160822 3413 17 47 36.8 -14 43 33 5.94 B9pHgMn G:Member of Pleiades group.,SB:12.4520d, K 52.5k/s, V0 -18.5k/s, asini 8.97.
HR 6666 BD-10 4560 162757 160885 17 53 03.6 -10 53 59 6.18 gK1
HR 6681 BD-15 4722 163336 160915 10891 17 56 19.0 -15 48 45 5.89 A1V 3.2 20.6 D:AB CPM; C, 12v at 34" optical.
HR 6710 ζ 57 BD-03 4217 164259 142025 18 00 29.0 -03 41 25 4.62 F2IV
HR 6755 BD-08 4558 165402 142083 3436 18 06 07.4 -08 19 26 5.85 B8III-IV G:Sco-Cen assoc.
HR 6756 BD-04 4395 165438 142085 18 06 15.2 -04 45 05 5.77 K1+IV
HR 6785 BD-13 4863 166103 161125 1472 I 18 09 43.4 -13 56 04 6.39 K0
HR 6813 BD-04 4415 166960 142159 3450 18 13 10.0 -04 00 42 6.59 A2m
HR 6830 BD-03 4259 167564 142185 18 15 58.0 -03 37 03 6.36 A4V
HR 6840 BD-03 4263 167768 142189 18 16 53.1 -03 00 26 6.00 G3III G:Arcturus group?
HR 6843 BD-09 4678 167833 142192 1475 18 17 24.2 -09 45 31 6.31 A8V
HR 6858 BD-15 4927 168415 161348 I 18 20 08.8 -15 49 54 5.39 K4III
HR 6869 η 58 BD-02 4599 168723 142241 688 I W 10675 18 21 18.6 -02 53 56 3.26 K0III-IV 8.7 179.7 S:Also classified K0III-IV.
HR 6873 BD+05 3704 168797 123385 10688 18 21 28.5 +05 26 09 6.13 B3Ve S:Shell star.,VAR:6.11 - 6.14V. Emission variable 12 to over 22 yrs.
HR 6890 BD-03 4277 169268 142274 18 24 03.5 -03 35 00 6.38 F6III-IV SB:Equal components.
HR 6898 BD-01 3486 169493 142294 11324 18 24 57.0 -01 34 46 6.15 F6III+A9III 0.4 0.8 D:6.8 F6III, 7.0 A7IV, 240y, a = 0.59". Combined mag., colors.
HR 6900 BD+05 3730 169578 123453 18 25 08.8 +05 05 05 6.74 B9V
HR 6918 59 BD+00 3936 169985 123497 11353 d Ser 18 27 12.5 +00 11 46 5.21 G0III+A6V 2.3 3.8 D:AB physical. B is F5V, vsini =<54k/s. Component P, vsini 80:k/s.,DYN:0.007".,SB:ADS 11353A is triple spectroscopic system with periods 385 and 1.8505205d. vsini of A-type component 270k/s, of G-type,,SB:80:k/s. Comp. B may also be SB, and third visual component P at 0.1" from A may be one of the components of the long,SB:period pair. ADS 11353A, 1.8505, K 90k/s, asini 2.29. ADS 11353Ap?, 386.0d, K 28k/s, V0 -23.3k/s, asini 731.,SB:Companion with sep. 0.25" seen only on 1976.61; unresolved at four other epochs between 1976.3 and 1979.5 (McAlister,SB:and Hartkopf).,SB:28k/s, V0 -23.3k/s, asini 731.,VAR:ADS 11353A, 4.9 - 5.9v.
HR 6928 BD+06 3790 170200 123516 S 18 27 58.8 +06 11 39 5.73 B8III-IV 0.1 G:Hyades group; NGC 6633 #102.,SB:3.4941d, K 38.5k/s, V0 -14.7k/s, asini 1.85. Mass loss from primary. If mass ejection discontinuous, mag. may,SB:remain constant over long intervals.
HR 6935 60 BD-02 4641 170474 142348 1480 18 29 41.0 -01 59 07 5.39 K0III SB:3.1558d, K 3.6k/s.
HR 6957 61 BD-01 3504 170920 142372 18 31 57.0 -01 00 11 5.94 A4III N:Some older catalogues following BAC call this e Ser. However, Heis and followers, including HR, call HR 6993 = e.
HR 6958 BD+03 3737 170973 123610 MV Ser 18 32 07.0 +03 39 35 6.43 A0pSiCr S:Magnetic star. Also classified B9.5IVp.,VAR:0.945099d, amp. 0.03U.
HR 6993 BD-00 3521 171978 142444 3480 11122 18 37 36.0 -00 18 34 5.75 A1V+A1V G:Sirius group? UMa stream; UMa cluster.,SB:14.674d, K 38.6k/s, V0 +11.4k/s, msin3i 0.319, asini 7.62, i 29d, vsini 26 and <26k/s.
HR 6999 BD-03 4331 172088 142461 11520 18 38 23.7 -03 11 37 6.49 F9IV 0.1 0.1 D:AB 7.2 F9V, 7.3 F9V, sep. 0.13", 12.18y, a = 0.196". Measured sep. 0.141" on 1985.5 by speckle interferometry. Third,D:component 14v, optical.,DYN:0.028".
HR 7000 BD-01 3529 172103 142460 18 38 19.1 -01 06 48 6.66 F1IV-V
HR 7008 BD+05 3891 172365 123778 3485 18 39 36.9 +05 15 51 6.38 F8Ib-II G:IC 4756 #145.,S:CNO content high relative to (Fe/H) and Lithium abundance high (at or near interstellar value).
HR 7048 BD+05 3941 173495 123886 11640 18 45 28.4 +05 29 59 5.83 A1V+A1V 0.3 1.3 D:ADS 11640AB, >5600y. Both components close binaries. Speckle interferometry 1985.5 gives sep. Aa = 0.141";,D:Bb = 0.137".,SB:ADS 11640A. A1, A4.
HR 7076 BD+04 3884 173954 123928 3494 I 18 48 02.7 +04 14 29 6.21 K5 v S:Profiles of H alpha and H beta emission vary.
HR 7141 θ1 63 BD+04 3916 175638 124068 709 11853 A 11557 18 56 13.2 +04 12 13 4.62 A5V 0.4 22.2 D:Binary with HR 7142.,DYN:0.019".,G:Hyades group.,N:Alya; Alga.,VAR:4.59 - 4.72V.
HR 7142 θ2 63 BD+04 3917 175639 124070 11853 B 18 56 14.6 +04 12 07 4.98 A5Vn 0.4 22.2 D:Binary with HR 7141.,DYN:0.019".
HR 7144 BD+02 3730 175679 124073 W 18 56 25.6 +02 28 16 6.15 G8III 5.7 100.
HR 7158 64 BD+02 3738 175869 124089 18 57 16.6 +02 32 07 5.57 B9IIIep:Hg: v G:Member of the local association (Pleiades group).,S:H alpha emission.,VAR:Hydrogen line widths vary in cycles of about 10 yrs.

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