Kataloge

Eridanus / 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 472 α CP-57 334 10144 232481 54 Var 01 37 42.9 -57 14 12 0.46 B3Vpe v G:Member of Pleiades group.,N:ACHERNAR.,R:Diam. = 0.00185 - 0.00192".,RV:Period in RV and light (1.26d) seems best explained by rotation. Weak but significant variations in strength of,RV:MgII 4481. RV of H gamma and HeI 4471 consistent with period, amp. 30k/s. Variable light amp. 0.02V.,S:Lyman alpha and Lyman beta observed from COPERNICUS. H alpha and H beta var. emission and possible high-velocity mass,S:loss. Expanding circumstellar shell.,VAR:EB or Ell, amp. 0.02V. H alpha var. emission and possible high-velocity mass loss. Expanding circumstellar shell.
HR 479 CP-54 358 10241 232483 W 01 38 48.2 -53 26 20 6.84 F5IV-V 1.3 10.4 D:CPM. Combined mag., colors. Primary F4IV-V, secondary F8V.,RV:Component B, -4k/s.
HR 486 CP-56 329 10360 232492 W B 01 39 47.4 -56 11 53 5.87 K0V 0.1 10.8 D:Binary with HR 487, q.v.,N:With HR 487 called p Eridani.
HR 487 CP-56 329 10361 232490 W A 01 39 47.8 -56 11 41 5.76 K5V 0.1 10.8 D:AB 5.79 K0V, 5.83 K0V, 483.66y, a = 7.817". B is HR 486. Combined light HR 486-487, 5.07V. Spectra also classified,D:K1V, K1.5V.,DYN:0.108".
HR 506 CP-54 365 10647 232501 01 42 29.3 -53 44 26 5.52 F9V
HR 520 CP-54 377 10939 232520 2118 01 46 06.3 -53 31 19 5.04 A1V
HR 566 χ CP-52 241 11937 232573 68 W 671 01 55 57.5 -51 36 32 3.70 G8IIIbCNIV 6.5 4.8 D:CPM.
HR 573 CP-52 242 12042 232581 01 57 00.1 -51 45 58 6.10 F6-7V
HR 637 CD-51 532 13445 232658 02 10 25.6 -50 49 28 6.12 K1V
HR 674 φ CP-52 285 14228 232696 82 W 02 16 30.6 -51 30 44 3.56 B8V-IV 5.0 87.6 C:Color excess E(B-V) = 0.00,D:Companion G2V?,G:Pleiades group.,S:Neutral carbon continuum shows discontinuities in UV.
HR 701 CD-51 571 14943 232736 02 22 54.6 -51 05 32 5.92 A5V
HR 721 κ CD-48 637 15371 215906 86 I 02 26 59.1 -47 42 14 4.25 B5IV G:Pleiades group.
HR 789 CD-43 814 16754 215996 2185 W 02 39 48.0 -42 53 30 4.75 A2V 10.0 23.8
HR 794 ι CD-40 689 16815 215999 1075 I 02 40 40.0 -39 51 20 4.11 K0III
HR 807 CD-47 832 17006 216013 2189 02 42 08.5 -46 31 28 6.10 K1III
HR 814 CD-41 769 17098 216019 W 02 43 20.3 -40 31 39 6.36 B9V 0.3 1.9 D:Binary. Combined mag., color.,RV:Both components 16k/s.
HR 818 τ1 1 BD-19 518 17206 148584 02 45 06.2 -18 34 21 4.47 F6V SB:958d, K 3.0k/s, V0 +3.0k/s, asini 35.3. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).
HR 822 CD-46 797 17325 216036 02 45 16.5 -46 17 14 6.85 K2III
HR 826 BD-22 479 17390 168045 02 46 45.2 -21 38 23 6.49 F3IV
HR 827 CD-23 1061 17438 168051 02 47 11.2 -22 29 08 6.47 F2
HR 832 BD-13 530 17491 148612 I Z Eri 02 47 56.0 -12 27 38 6.90 M4III v G:Wolf 630 group.,VAR:SRb 7.0 - 8.63p, 80d. Secondary cycle 746d.
HR 850 τ2 2 BD-21 509 17824 168094 102 I 2179 02 51 02.3 -21 00 15 4.75 K0III 10.2 46.7 N:Angetenar; Al Anchat al Nahr; Anchat.
HR 853 CD-40 736 17864 216065 02 50 47.9 -39 55 54 6.36 A0V
HR 857 BD-13 544 17925 148647 975 02 52 32.1 -12 46 10 6.04 K2V
HR 859 BD-10 569 17943 130160 02 52 50.5 -09 26 28 6.32 A7IV N:Bayer's Sigma Eri in this position: no Sigma found in any other source.
HR 862 BD-22 503 18071 168121 02 53 35.3 -22 22 35 5.95 K0III S:IR spectra show water vapor.
HR 874 η 3 BD-09 553 18322 130197 104 I 988 02 56 25.7 -08 53 53 3.89 K1-IIIbBa0.2: G:Wolf 630 group.,N:Azha.
HR 875 BD-04 502 18331 130199 1080 02 56 37.4 -03 42 44 5.17 A1Vn G:UMa stream.
HR 883 4 CD-24 1336 18454 168183 02 57 23.7 -23 51 43 5.45 A5V
HR 889 6 CD-24 1343 18535 168191 I 02 58 05.7 -23 36 22 5.84 K2III
HR 892 BD-03 470 18543 130215 W 02 58 42.0 -02 46 57 5.23 A2IV 7.3 2.7
HR 895 BD-10 585 18557 130216 02 58 47.4 -09 46 35 6.14 A2m
HR 897 θ1 CD-40 771 18622 216113 106 W A 1002 02 58 15.7 -40 18 17 3.24 A4III 1.1 8.3 D:Binary with HR 898. Uncertain which component var. Combined mag. HR 897/8, 2.91V; combined colors, +0.125(B-V),,D:+0.13(U-B).,DYN:0.016".,N:ACAMAR.
HR 898 θ2 CD-40 771 18623 216114 W B 1002 02 58 16.3 -40 18 16 4.35 A1V 1.1 8.3 D:Binary with HR 897.,DYN:0.016".
HR 899 5 BD-03 475 18633 130228 2209 1008 02 59 41.2 -02 27 54 5.56 B9.5V
HR 904 7 BD-03 478 18760 130242 I CV Eri 03 00 51.0 -02 52 43 6.11 M1III VAR:Lb? 6.11 - 6.29V.
HR 907 ρ1 8 BD-08 562 18784 130243 03 01 10.0 -07 39 46 5.75 K0II S:Strong CN.
HR 912 BD-10 594 18885 148721 2216 03 01 56.1 -09 57 41 5.83 gG6
HR 913 BD-07 537 18894 130251 03 02 09.3 -06 29 41 6.19 G0IV-V SB:F8V+G5V, 363.10d, K1 24k/s, K2 30k/s, V0 +16.18k/s, a1sini 87, a2sini 108.8.
HR 917 ρ2 9 BD-08 568 18953 130254 I 2312 1024 03 02 42.3 -07 41 07 5.32 K0II-III 4.2 1.9 D:CPM.,S:Strong CN.,VAR:ADS 2312B, 8.5 - 11.0v.
HR 919 τ3 11 CD-24 1387 18978 168249 1085 03 02 23.5 -23 37 28 4.09 A4IV G:UMa stream.
HR 925 ρ3 10 BD-08 572 19107 130269 03 04 16.4 -07 36 03 5.26 A8V
HR 929 CD-47 932 19141 216150 1086 03 02 55.9 -46 58 30 5.82 K2-3III
HR 935 BD-06 606 19349 130284 2221 I W 03 06 33.5 -06 05 19 5.27 M3III 7.2 15.9
HR 953 CD-24 1480 19826 168354 03 10 35.4 -23 44 18 6.38 K0IV
HR 955 BD-04 540 19836 130328 2224 I 2389 03 11 18.8 -03 48 42 6.05 M1III 5.9 24.4 D:Optical.
HR 957 BD-16 587 19887 148821 03 11 16.8 -16 01 31 6.26 K0
HR 968 CD-44 1025 20121 216209 2228 W 03 12 25.8 -44 25 11 5.93 F7III+A0V 0.4 0.2 D:AB 6.6 G2III, 6.9 A7IV, 44.82y, a = 0.443". Combined mag., colors. Component C 9.5v at 3" physical.,S:Primary variously classified F4III, F6III, F3V, F5V, even G2III.
HR 983 BD-06 636 20319 130388 2440 1090 03 16 00.9 -05 55 07 6.17 B9V 0.2 0.9 DYN:0.003".,VAR:ADS 2440. B-A varies from 0.2 to 2.0m. Uncertain which component varies. B6, A1.
HR 984 ζ 13 BD-09 624 20320 130387 1091 1088 03 15 50.0 -08 49 11 4.80 A5m N:Zibal in Becvar, but this does not correspond to the position of Al Zibal (in Phoenix) described by Allen.,SB:17.922d, K 18.8k/s, V0 -4.5k/s, asini 4.40.
HR 988 14 BD-09 627 20395 130395 03 16 35.7 -09 09 16 6.14 F1V
HR 994 15 BD-22 1146 20610 168452 I 2463 03 18 22.1 -22 30 41 4.88 G6III 1.3 0.2 DYN:0.004".,N:CoD-22d1146 = CPD-22d 349; south of -23d at epoch 1855, but in Southern Durchmusterung extension as SD-23d 44.,VAR:Considered variable by Gould, but never confirmed.
HR 997 BD-19 651 20631 148897 2465 03 18 41.2 -18 33 35 5.71 F0IV 2.3 7.2 D:Binary.,DYN:0.034".,SB:ADS 2465A.
HR 1003 τ4 16 BD-22 584 20720 168460 I 2472 Tau4 Eri 03 19 31.0 -21 45 28 3.69 M3.5IIIaCa-1 e 6.2 5.5 D:AB binary, B is K0V. C, 11v at 40" optical.,DYN:0.010".,G:Hyades group.,S:Ultraviolet FeII emission.,VAR:Lb? 3.57 - 3.72V.
HR 1008 CD-43 1028 20794 216263 119 I 03 19 55.7 -43 04 11 4.27 G8V S:Also classified G8III.
HR 1016 CD-24 1600 20894 168482 03 21 24.0 -23 38 07 5.52 G6.5IIbCN-1Hdel -1 G:Sirius group; UMa stream.
HR 1024 BD-08 643 21019 130457 2507 03 23 17.8 -07 47 39 6.20 G2V 6.4 3.9 D:Binary.,DYN:0.043".
HR 1049 CD-42 1115 21473 216316 03 26 11.7 -41 38 13 6.32 A0V
HR 1050 BD-11 667 21530 148972 03 28 01.0 -11 17 12 5.73 K2III
HR 1060 BD-07 606 21665 130520 03 29 39.1 -06 48 18 5.99 G5
HR 1062 BD-13 662 21688 148985 2246 03 29 36.0 -12 40 29 5.59 A5IV
HR 1070 17 BD-05 674 21790 130528 1097 03 30 37.1 -05 04 31 4.73 B9V s
HR 1075 CD-43 1085 21882 216347 03 29 55.0 -42 38 03 5.78 A5V
HR 1076 CD-41 1029 21899 216350 2248 1179 03 30 13.6 -41 22 12 6.12 F7V
HR 1084 ε 18 BD-09 697 22049 130564 127 I A 03 32 55.8 -09 27 30 3.73 K2V 3.0 2.0 D:Astrometric binary, 25y. Unresolved by speckle interferometry.
HR 1088 τ5 19 BD-22 628 22203 168634 1099 03 33 47.3 -21 37 58 4.27 B8V+B8V G:Pleiades group.,SB:6.2236d, K 107k/s, V0 +15.0k/s, msin3i 2.76, asini 8.97. Nearly equal components. vsini of secondary 39k/s.
HR 1091 BD-10 704 22243 149047 03 34 37.4 -09 52 07 6.25 A2V
HR 1098 BD-11 696 22409 149057 03 35 57.7 -11 11 37 5.57 gG7
HR 1100 20 BD-17 699 22470 149063 1100 EG Eri 03 36 17.4 -17 28 01 5.23 B9.5p G:Pleiades group.,S:Lambda Boo star, Ca, Mg 4481 wk. Formerly classified B9pSi, helium-weak.,VAR:5.23 - 5.32V, amp. 0.11U, 1.93d.
HR 1106 CD-40 1008 22663 216405 130 03 37 05.7 -40 16 29 4.58 K1III
HR 1108 BD-07 647 22675 130628 03 38 29.2 -07 23 30 5.85 gG5
HR 1111 21 BD-06 713 22713 130634 03 39 01.1 -05 37 34 5.96 K1V
HR 1116 BD-03 591 22798 130639 03 39 38.3 -03 23 35 6.23 G5
HR 1117 BD-10 717 22799 149082 03 39 25.4 -10 26 14 6.19 G5
HR 1120 BD-15 634 22905 149094 2259 03 40 11.4 -15 13 36 6.33 G5
HR 1121 22 BD-05 715 22920 130652 2260 03 40 38.3 -05 12 38 5.53 B9IIIpSi4200 S:Helium very weak.
HR 1125 BD-12 689 23010 149107 W 03 41 13.8 -11 48 11 6.49 F5II 7.7 14.7 G:Hyades group.
HR 1128 BD-20 687 23055 149114 03 41 22.4 -19 35 05 6.59 A3V
HR 1136 δ 23 BD-10 728 23249 130686 135 I Del Eri 03 43 14.9 -09 45 48 3.54 K0+IV e N:Rana in Becvar. But see HR 188.,S:CaII H and K emission.,VAR:RS:, 3.51 - 3.56V, about 10d.
HR 1139 BD-10 729 23281 149132 03 43 33.8 -10 29 08 5.60 A5m
HR 1143 CD-37 1415 23319 194475 2265 W 03 42 50.1 -37 18 49 4.59 K2.5III 7.6 5.4
HR 1146 24 BD-01 526 23363 130698 137 03 44 30.5 -01 09 47 5.25 B7V
HR 1150 25 BD-00 593 23413 130704 I 03 44 56.5 -00 17 48 5.55 K4III G:Zeta Her group.
HR 1157 CD-41 1119 23508 216459 W 03 44 06.2 -40 39 37 6.45 K1III 3.0 5.1 D:CPM. Primary K1IIIab, secondary G3IV.,G:Wolf 630 group.
HR 1162 π 26 BD-12 707 23614 149158 I Pi Eri 03 46 08.5 -12 06 06 4.42 M2III VAR:Lb? 4.38 - 4.44V.
HR 1173 τ6 27 CD-23 1565 23754 168827 140 03 46 50.9 -23 14 59 4.23 F3III
HR 1181 τ7 28 CD-24 1877 23878 168836 Var 03 47 39.6 -23 52 29 5.24 A2 VAR:Amp. 0.012u, about 7.17d.
HR 1182 BD-00 602 23887 111433 2273 03 48 38.9 +00 13 40 5.91 K3III
HR 1186 CD-36 1453 23958 194537 03 47 49.6 -36 06 21 6.21 B8V
HR 1187 BD-21 703 23978 168851 I 03 48 35.8 -20 54 11 5.81 K5III
HR 1189 CD-38 1297 24071 194550 W B 03 48 35.4 -37 37 20 5.40 A1V 0.6 8.0 D:Binary with HR 1190.,DYN:0.032".
HR 1190 CD-38 1297 24072 194551 W A 1359 03 48 35.9 -37 37 14 4.73 B9V 0.6 8.0 D:Binary with HR 1189.,DYN:0.032".
HR 1195 CD-36 1467 24160 194559 143 I 03 49 27.3 -36 12 01 4.17 G9II-III G:In Ursa cluster; Sirius group?
HR 1200 CD-36 1476 24305 194570 03 50 37.6 -36 25 31 6.86 B9.5V
HR 1202 30 BD-05 769 24388 130789 2832 03 52 41.6 -05 21 41 5.48 B8V 6.7 8.3 D:Companion F4V, optical.
HR 1206 BD-18 691 24497 149229 2276 03 53 13.0 -18 26 04 6.22 gK+F S:There is considerable confusion as to the classification of this binary. The HR catalogue (1908) gave G5; HD, F2 (the,S:most widely quoted); others gave F7V, F8V, A2: + K, and lastly (Bidelman) gK + F. If the given B-V is correct, the,S:gK + F is the most probable.
HR 1211 32 BD-03 631 24554 130805 2850 B 03 54 17.4 -02 57 10 6.14 A2V 1.5 6.8 D:Binary with HR 1212. C, 10v at 165".,DYN:0.006".
HR 1212 32 BD-03 631 24555 130806 I 2850 A 03 54 17.5 -02 57 17 4.79 G8III 1.5 6.8 D:Binary with HR 1211.,DYN:0.006".
HR 1213 τ8 33 CD-24 1945 24587 168925 Tau8 Eri 03 53 42.6 -24 36 45 4.65 B6V
HR 1214 CD-35 1455 24626 194608 2278 03 53 38.9 -34 43 56 5.11 B6V
HR 1217 BD-12 752 24712 149251 DO Eri 03 55 16.3 -12 05 57 6.00 A5pSrCrEu v S:Possibly the coolest magnetic star known, about 7000K. Variously classified Ap to F0pSr.,VAR:Alpha CV 5.97 - 6.00V, 12.4580 or 12.4564d. Rotation and magnetic field same period, no polarity reversal. Spectrum,VAR:variable, 12.460d. Maximum intensity Eu at minimum light.
HR 1219 CD-40 1128 24744 216546 2280 W 1414 03 54 23.2 -40 21 26 5.71 K0III+A3V 0.0 0.1 D:AB combined mag. and color. C, 12.7v at 23".
HR 1225 BD-10 793 24832 130833 2284 DL Eri 03 56 37.9 -09 45 03 6.19 F1V VAR:Delta Sct 6.17 - 6.24V, 0.155879d.
HR 1231 γ 34 BD-13 781 25025 149283 149 I 2904 Gam Eri 03 58 01.8 -13 30 31 2.95 M0.5IIICa-1Cr-1 e 9.5 52.8 N:Zaurak; Zaurac; Zaurack.,S:Ultraviolet FeII emission. Also classified M0.5III-IIIb Ca-1 Cr-1.,VAR:2.88 - 2.96V.
HR 1232 BD-05 789 25069 130860 03 58 52.3 -05 28 12 5.83 G9V
HR 1235 BD-12 766 25165 149299 I 03 59 30.1 -12 34 27 5.60 K5III
HR 1240 τ9 36 CD-24 2022 25267 169017 2287 Tau9 Eri 03 59 55.5 -24 00 59 4.66 B6V+B9.5V S:Also classified A0pSi.,SB:5.9537d, K 37.6k/s, V0 +24.9k/s, asini 3.06.,VAR:Alpha CV 4.62 - 4.67V, 1.2094d.
HR 1244 35 BD-01 572 25340 130878 1111 04 01 32.0 -01 32 59 5.28 B5V G:Member of the local association (Pleiades group); in HII region; Cas-Tau OB1.
HR 1246 CD-30 1597 25371 194689 2289 04 00 40.7 -30 29 27 5.93 A2V
HR 1249 BD-00 632 25457 130893 04 02 36.7 -00 16 08 5.38 F5V
HR 1258 BD-20 769 25631 169071 Var? 04 03 24.7 -20 08 39 6.46 B2.5V G:Member of the local association (Pleiades group).,VAR:Beta C amp. 0.04b, over 1d?
HR 1259 BD-20 770 25661 169078 04 03 36.8 -20 09 30 7.01 K2II
HR 1263 BD-16 770 25700 149345 2293 04 04 08.7 -16 35 20 6.39 K2
HR 1265 BD-13 806 25723 149351 04 04 22.7 -12 47 33 5.61 gK0
HR 1267 BD-20 774 25803 169095 04 04 41.0 -20 22 54 6.13 K0
HR 1272 BD-09 811 25910 130948 2294 04 05 56.5 -08 51 22 6.26 A3V
HR 1274 BD-20 780 25944 169111 04 05 46.7 -20 30 44 6.34 G5
HR 1275 CD-27 1540 25945 169110 153 04 05 37.4 -27 39 06 5.59 F1IV
HR 1288 BD-16 796 26326 149412 04 09 17.8 -16 23 09 5.37 B4V
HR 1290 37 BD-07 758 26409 131001 04 10 22.5 -06 55 26 5.44 G8III
HR 1293 BD-09 837 26464 131005 04 10 47.7 -08 49 11 5.70 gG9
HR 1298 ο1 38 BD-07 764 26574 131019 154 Omi1 Eri 04 11 51.9 -06 50 15 4.04 F2II-III N:Beid.,VAR:Delta Sct 4.00 - 4.05V, 0.0815d. Secondary per. 0.1291d.
HR 1299 CD-35 1588 26575 194810 04 10 45.8 -35 16 26 6.44 K1+IIIaCH-1.5 S:Weak G-band. Also classified G8III-IV.
HR 1300 BD-20 801 26591 169206 2302 04 11 36.2 -20 21 22 5.79 A2m SB:3.6587d, K 104.5k/s, V0 +32.8k/s, msin3i 1.75, asini 5.26. Two equal Am stars. Same vsini 30k/s.
HR 1312 BD-01 600 26739 131041 2305 04 13 38.2 -01 08 59 6.44 B5IV
HR 1318 39 BD-10 867 26846 149478 I 3079 04 14 23.7 -10 15 23 4.87 K3III 3.7 6.4 D:AB binary, B is G2V.,DYN:0.016".,G:Wolf 630 group.
HR 1325 ο2 40 BD-07 780 26965 131063 I 3093 DY Eri 04 15 16.3 -07 39 10 4.43 K1-V 5.0 83.4 D:BC 9.51 A2, 11.18 M4Ve, 252.1y, a = 6.943". Component B is white dwarf. Component A, CPM.,DYN:0.199".,N:Keid; Kied.,VAR:ADS 3093C; UV, min. 11.18V, +1.50 (B-V), 12.16 - 13.85U. X-ray source.
HR 1332 BD-06 862 27179 131092 04 17 19.2 -06 28 19 5.94 gG8
HR 1345 BD-21 831 27362 169317 I 1548 04 18 15.9 -20 42 56 6.00 G8III VAR:Amp. 0.3V.
HR 1347 υ4 41 CD-34 1614 27376 194902 W Var 04 17 53.7 -33 47 54 3.56 B9V 1.0 0.2 D:C, 11.8v at 49".,G:Member of Pleiades group.,S:HgMn star.,SB:B8, B9.5 5.0105d, K 63.8k/s, V0 +17.8k/s, msin3i 0.559, asini 4.40. Equal components, equal vsini 12k/s;,SB:rotational velocity 31k/s.,VAR:Small amp., possible periods 0.96, 1.93, 8.5, 0.89d, with 8.5 slightly favored (Manfroid and Mathys 1985, A&AS,,VAR:59, 429).
HR 1353 CD-23 1856 27411 169325 04 18 37.4 -22 58 13 6.07 Am S:K/H/m indicate A4/F0/F5, respectively.
HR 1359 CD-34 1626 27490 194923 W A 04 19 03.0 -33 54 18 6.37 A3V 2.1 6.0 D:Secondary F7V, vsini 90k/s.
HR 1362 BD-06 875 27536 131129 EK Eri 04 20 38.7 -06 14 44 6.27 G8IV: VAR:BY, amp. 0.12V, 154d.
HR 1363 BD-07 798 27563 131132 2322 EM Eri 04 20 42.8 -07 35 33 5.85 B5III VAR:Varies several hundredths of a mag. on a time scale of days.
HR 1366 BD-00 687 27611 131140 I 3152 04 21 27.1 -00 05 53 5.86 K3III 5.0 197.8 D:B, 13.0v at 36" optical.
HR 1367 BD-20 831 27616 169354 161 04 20 39.0 -20 38 23 5.38 A2V
HR 1374 CD-26 1642 27710 169368 3159 AB 1574 04 21 31.3 -25 43 42 6.01 F0IV-V 0.3 0.6 D:AB 6.6 F1V, 6.9 F3V, 76.92y, a = 0.500". Combined mag., color. Component C, 12v at 37" optical; D, 8.25V, +0.57(B-V),,D:+0.04(U-B), G0 at 45" CPM.,DYN:0.019".,VAR:Amp. 0.13V.
HR 1383 ξ 42 BD-04 818 27861 131176 1120 1590 04 23 40.8 -03 44 44 5.17 A2V G:In Ursa cluster? Sirius group; UMa stream.,VAR:Delta Sct?
HR 1384 CD-25 1862 27881 169391 2323 I 1588 04 23 05.7 -24 53 32 5.83 K5 VAR:Amp. 0.12V.
HR 1386 CD-35 1687 27941 194971 W 04 23 07.7 -35 32 42 6.39 K1III 7.0 18.7
HR 1393 43 CD-34 1664 28028 194984 1121 04 24 02.2 -34 01 01 3.96 K4III G:Hyades group.
HR 1398 CD-35 1704 28143 194996 W 04 24 56.4 -34 45 28 6.55 F2III 3.4 39.5 D:AB optical? C, 11v at 4" from B.
HR 1410 CD-24 2343 28312 169455 3230 04 26 57.0 -24 04 53 6.11 A2 0.2 0.4 D:6.8 A2, 7.0, 175.7y, a = 1.250".
HR 1421 BD-19 931 28479 149668 04 28 39.0 -19 27 30 5.96 K1III
HR 1423 BD-13 893 28497 149674 2332 DU Eri 04 29 06.9 -13 02 54 5.60 B1Vne v S:Lyman beta observed from COPERNICUS. Expanding circumstellar shell.,VAR:Gamma Cas 5.41 - 5.49V. Expanding circumstellar shell; possibly high velocity mass loss. Equivalent width of H alpha,VAR:variable.
HR 1431 BD-13 896 28625 149682 04 30 09.7 -13 35 32 6.24 G5
HR 1437 45 BD-00 713 28749 131270 I 04 31 52.7 -00 02 38 4.91 K3II-III
HR 1438 BD-13 904 28763 149702 3284 04 31 25.9 -13 38 42 6.21 A3V 3.2 29.1
HR 1439 CD-35 1768 28776 195085 2334 W 04 30 40.3 -35 39 13 5.96 K0II 8.3 36.6
HR 1441 BD-03 809 28843 131279 W DZ Eri 04 32 37.4 -03 12 33 5.81 B9III v 3.4 124.5 S:He weak.,VAR:SX Ari 5.73 - 5.82y, 1.374d. Var. helium lines.
HR 1447 BD-11 900 28970 149725 I 04 33 22.0 -10 47 09 6.06 K0
HR 1449 46 BD-07 838 29009 131309 3305 EH Eri 04 33 54.8 -06 44 20 5.72 B9pSi 4.8 1.2 D:CPM.,VAR:Alpha CV, amp. 0.035V, 0.065U, 3.80d.
HR 1450 BD-07 841 29063 131317 I 04 34 14.2 -06 50 16 6.09 K2III
HR 1451 47 BD-08 887 29064 131315 2337 I DV Eri 04 34 11.6 -08 13 53 5.11 M3III VAR:Lb? 5.10 - 5.13V, amp. 0.20p.
HR 1452 BD-09 930 29065 131316 I 04 34 11.7 -08 58 13 5.26 K4III
HR 1453 υ1 50 CD-30 1883 29085 169570 I 1650 04 33 30.6 -29 46 00 4.51 K0IIICN-1
HR 1460 BD-10 959 29173 131335 3318 A 04 35 14.0 -09 44 12 6.37 A1m 1.0 12.8 D:CPM. Companion A7V.
HR 1461 BD-20 880 29184 169584 04 35 00.5 -19 55 14 6.13 K3III
HR 1462 BD-03 830 29227 131344 3328 04 36 01.6 -03 36 43 6.33 B7III 4.7 17.9 D:Component C optical.
HR 1463 ν 48 BD-03 834 29248 131346 169 W Nu Eri 04 36 19.1 -03 21 09 3.93 B2III 9.2 50.9 G:Ori OB1.,RV:0.19d.,VAR:Beta C 3.4 - 3.60p, 0.17790414d, changing. Probable interference periods 0.1779 and 0.1735d with beat period of,VAR:7.0256d. Possibly also E, 103.9d.
HR 1464 υ2 52 CD-30 1901 29291 195148 170 I 04 35 33.0 -30 33 44 3.82 G8IIIa N:Theemim; Beemin. Allen applies this name, after Bayer, to the series of stars, Upsilon1 through Upsilon7,N:Eri, or HR 1143, 1195, 1214, 1347, 1393, 1453 and 1464. (The order of the superscripts varies among different,N:catalogues.),S:Also classified G8IIIa.
HR 1474 51 BD-02 963 29391 131358 3350 04 37 36.1 -02 28 24 5.23 F0V 5.9 80.0 D:IDS gives AB, 5.3, 11.8v sep. 30". Optical. Component C by Wallenquist.
HR 1476 CD-30 1911 29435 195163 04 36 50.9 -30 43 00 6.30 B9IV-V
HR 1481 53 BD-14 933 29503 149781 172 I W 04 38 10.8 -14 18 14 3.87 K2IIIb 3.4 0.8 N:Sceptrum.
HR 1483 BD-12 955 29573 149789 04 38 53.6 -12 07 23 5.01 A2IV
HR 1487 BD-14 936 29613 149797 04 39 19.7 -14 21 33 5.45 K1IVa
HR 1488 BD-01 689 29610 131392 04 39 47.2 -01 03 10 6.10 K0
HR 1495 CD-24 2488 29737 169650 1127 04 40 06.8 -24 28 57 5.58 G6III
HR 1496 54 BD-19 988 29755 149818 I 3380 DM Eri 04 40 26.5 -19 40 18 4.32 M4III 0.3 0.1 D:Seen as double only in 1877 and 1923.,VAR:SRb 4.28 - 4.36V, 30d.
HR 1505 55 BD-09 969 30020 131442 3409 B DW Eri 04 43 34.6 -08 47 37 6.82 F4IIIpSr 0.1 9.3 D:CPM with HR 1506.,VAR:Alpha CV?, amp. 0.025V.
HR 1506 55 BD-09 970 30021 131443 3409 A 04 43 35.1 -08 47 46 6.70 G8III 0.1 9.3 D:CPM with HR 1505.
HR 1508 56 BD-08 929 30076 131451 1131 DX Eri 04 44 05.3 -08 30 13 5.90 B2Ve RV:Pole on.,VAR:Gamma Cas 5.76 - 5.98V. Equivalent width of H alpha is variable. Amp. 0.09R, 0.05(R-I).
HR 1513 BD-18 906 30127 149856 2352 04 44 08.0 -18 40 00 5.53 A3V
HR 1520 μ 57 BD-03 876 30211 131468 176 04 45 30.1 -03 15 17 4.02 B5IV G:Member of the local association (Pleiades group); Cas-Tau OB1.,SB:B3, A3, 7.3589d, K 19.4k/s, V0 +23.3k/s, asini 1.90.
HR 1521 BD-21 966 30238 169727 I 04 45 04.2 -21 17 01 5.72 gK2
HR 1525 CD-28 1735 30422 169752 1132 04 46 25.8 -28 05 15 6.19 A3IV
HR 1532 58 BD-17 954 30495 149888 04 47 36.3 -16 56 04 5.51 G2.5V S:Also classified G2.5V.
HR 1536 BD-05 1044 30562 131504 04 48 36.3 -05 40 26 5.78 F8V G:Eta Cep group.
HR 1538 59 BD-16 956 30606 149901 04 48 32.5 -16 19 46 5.77 F6V
HR 1545 BD-14 970 30743 149916 2363 04 49 42.2 -13 46 11 6.26 F5V
HR 1549 60 BD-16 964 30814 149924 I 1740 04 50 11.6 -16 13 02 5.03 K0III v
HR 1560 ω 61 BD-05 1068 31109 131568 2366 04 52 53.7 -05 27 10 4.39 F4III+A6III SB:3057d, K 18.1k/s, V0 -8.3k/s, asini 676. Massive invisible component may be a black hole. Unresolved by speckle,SB:interferometry 1980.02.
HR 1579 BD-16 991 31414 149985 04 55 06.8 -16 44 26 5.70 gG9
HR 1581 BD-16 992 31444 149988 2370 R Eri 04 55 18.6 -16 25 04 5.72 gG4 VAR:Cst? 5.72V.
HR 1582 62 BD-05 1091 31512 131614 W 04 56 24.2 -05 10 17 5.51 B6V 3.6 67.3
HR 1595 BD-14 1003 31726 150029 04 57 44.8 -14 13 53 6.15 B1V
HR 1608 63 BD-10 1066 32008 150060 2375 04 59 50.4 -10 15 48 5.38 G4V
HR 1611 64 BD-12 1047 32045 150064 S Eri 04 59 55.8 -12 32 15 4.79 F0IV VAR:RRc 4.77 - 4.80V, 0.273d.
HR 1614 BD-05 1123 32147 131688 05 00 49.0 -05 45 12 6.22 K3V
HR 1617 ψ 65 BD-07 948 32249 131700 05 01 26.3 -07 10 26 4.81 B3V
HR 1625 BD-04 1019 32393 131715 05 02 45.5 -04 12 35 5.85 K3 S:Probably not a supergiant but may be composite.
HR 1657 66 BD-04 1044 32964 131777 3698 1831 05 06 45.7 -04 39 18 5.12 B9V+A1V 5.4 52.8 SB:B9.5, B9.5, 5.5227d, K 103.8k/s, V0 +32.6k/s, msin3i 2.38, asini 7.85. Nearly equal components; secondary is,SB:the more massive, a mercury star. vsini of both components =<41k/s.,VAR:E? 5.1 - 5.6v. About 2d.
HR 1666 β 67 BD-05 1162 33111 131794 188 I W 1841 05 07 51.0 -05 05 11 2.79 A3III 8.0 116.7 G:Sirius group; UMa stream.,N:Cursa; Dhalim; Kursa.
HR 1671 BD-08 1037 33224 131806 3722 A 05 08 20.2 -08 39 54 5.78 B8V 3.2 21.6 D:ADS 3722B, K0III-IV, RV +72k/s.
HR 1673 68 BD-04 1056 33256 131813 05 08 43.6 -04 27 22 5.12 F2V
HR 1679 λ 69 BD-08 1040 33328 131824 190 Lam Eri 05 09 08.8 -08 45 15 4.27 B2IVne v M:Candidate for becoming a Be star.,RV:0.701538d. Amp. varies 30 to 60k/s on time scale of a year or less, correlated with hydrogen emission. Possibly,RV:pulsating.,S:Shell star. H alpha emission with variable profile. Also classified B2III(e)p.,VAR:Beta C 4.22 - 4.34V, 0.701538d. Both spectroscopic and new photometric data suggest period 0.70177d. Small changes in,VAR:mean brightness (<0.1mag).

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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