Kataloge

Pegasus / 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 4 86 BD+12 5063 87 91701 2004 00 05 42.0 +13 23 46 5.51 G5III
HR 19 BD+24 3 417 73769 00 08 52.2 +25 27 46 6.23 K0III
HR 22 87 BD+17 7 448 91734 00 09 02.4 +18 12 43 5.53 G9III
HR 39 γ 88 BD+14 14 886 91781 7 I W Gam Peg 00 13 14.2 +15 11 01 2.83 B2IV 8.9 163.4 C:Color excess E(B-V) = +0.01.,N:ALGENIB.,RV:RV also varies with period 0.151750125d.,S:Lyman beta observed from COPERNICUS. Chlorine in spectrum.,SB:6.830713d, K 1.34k/s, V0 2.5k/s, asini 0.181Solar R.,VAR:Beta C 2.80 - 2.87V, 0.1517495d.
HR 45 χ 89 BD+19 27 1013 91792 1004 I 99 00 14 36.2 +20 12 24 4.80 M2+III e S:Ultraviolet FeII emission.,VAR:4.78 - 4.86V.
HR 49 BD+21 13 1048 73838 00 14 56.1 +22 17 03 6.24 A1pSi G:Pleiades group.
HR 8116 BD+15 4375 202128 106930 14761 21 13 28.8 +15 58 57 6.27 A7Vn 0.1 0.2 D:7.0 A7V, 7.0 A7V, 34.44y, a = 0.227". Combined mag., colors. Measured sep. 0.090" on 1985.5 by speckle interferometry.,DYN:0.014".
HR 8165 BD+23 4294 203344 89640 3704 21 21 04.4 +23 51 21 5.57 K1III G:Eta Cep group.,N:34 Vul in Peg. Very close to boundary.
HR 8173 1 BD+19 4691 203504 107073 804 I 14909 21 22 05.2 +19 48 16 4.08 K1III 4.9 36.2 D:AB CPM. Companion K0V.,SB:ADS 14909B.
HR 8210 BD+18 4794 204188 107138 IK Peg 21 26 26.7 +19 22 32 6.07 A8m SB:21.724d, K 41.5k/s, V0 -12.4k/s, asini 12.4.,VAR:Delta Sct amp. 0.01V, 0.044d.
HR 8219 BD+07 4696 204445 126818 1564 I 13727 21 28 24.8 +08 11 44 6.40 M1 VAR:Amp. 0.06V.
HR 8221 BD+17 4592 204560 107168 13738 21 28 59.9 +17 54 21 6.44 K5
HR 8223 BD+21 4555 204585 89737 I W 13740 21 28 59.9 +22 10 46 5.93 M4.5III-IIIa 2.7 41.1
HR 8225 2 BD+23 4325 204724 89752 1565 I 15027 21 29 56.9 +23 38 20 4.57 M1+III 8.1 29.8
HR 8231 BD+11 4583 204862 107195 21 31 09.6 +12 08 15 6.08 B9.5V
HR 8240 BD+22 4418 205087 89786 13774 21 32 27.1 +23 23 40 6.70 B9pSiSrCr
HR 8250 BD+22 4431 205420 89807 21 34 34.0 +22 45 17 6.47 F7V
HR 8257 BD+27 4107 205539 89815 S 21 35 19.0 +28 11 50 6.31 F0IV 0.2 SB:12.21d, K 52.0k/s, V0 -43.2k/s, msin3i 0.966, asini 8.27.
HR 8258 BD+23 4346 205541 89819 15115 21 35 27.0 +24 27 08 6.11 A4V 0.3 0.3 D:6.7 A2V, 7.0 A4V, 173.9y, a = 0.293". Combined mag. A third component is suspected.,DYN:0.008".
HR 8265 3 BD+05 4830 205811 126940 15147 A 21 37 43.7 +06 37 06 6.18 A2V 1.5 39.2 D:AB CPM. B is 7.65V, +0.37(B-V), -0.01(U-B), F2V; vsini 30k/s.,SB:SB = occultation binary unresolved by speckle interferometry.
HR 8267 5 BD+18 4827 205852 107288 1570 21 37 45.4 +19 19 07 5.45 F1IV VAR:Delta Sct?
HR 8270 4 BD+05 4834 205924 126956 15157 21 38 31.9 +05 46 18 5.67 A9IV-Vn 6.4 27.2 D:Optical.
HR 8274 BD+24 4445 206027 89870 S 21 38 45.0 +25 29 56 6.16 G9III 0.1
HR 8276 BD+19 4754 206043 89871 21 39 01.1 +20 15 55 5.85 F2V
HR 8289 7 BD+05 4850 206487 127002 3732 I 13848 21 42 15.5 +05 40 48 5.30 M2IIIab
HR 8292 BD+10 4604 206540 107340 21 42 33.0 +10 49 29 6.09 B5IV
HR 8308 ε 8 BD+09 4891 206778 127029 815 I 15268 Eps Peg 21 44 11.2 +09 52 30 2.39 K2Ib e 6.1 142.5 C:Large infrared excess.,D:ADS 15268AB optical.,G:See HR 8232.,N:ENIF; Enf; Enir; Al Anf; Os Pegasi; Fom.,S:Ultraviolet FeII emission. MgII emissions indicate a cooler shell surrounding the supergiant. Barium marginally,S:overabundant.,VAR:0.7 - 3.5V. 1.7m flare 1972 Sept. 26-7; fainter than normal following night.
HR 8313 9 BD+16 4582 206859 107365 I 13864 21 44 30.7 +17 21 00 4.34 G5Ib
HR 8314 BD+14 4668 206860 107364 3737 HN Peg 21 44 31.3 +14 46 19 5.94 G0V v VAR:Amp. 0.02V, 24.90d. Var. due to star spots? Period corresponds to period of rotation. Variable H and K emission,VAR:indicates chromospheric activity.
HR 8315 κ 10 BD+24 4463 206901 89949 I 15281 21 44 38.7 +25 38 42 4.13 F5IV 0.4 0.3 D:AB 4.7 F2IV, 5.0 F6IV, 11.558y, a = 0.255". ADS 15281C, 10.8v at 13.8" possibly in hyperbolic orbit about AB or is,D:optical.,DYN:0.024".,SB:ADS 15281B, 5.97152d, K 34.2k/s, V0 -5.7k/s, asini 2.803. ADS component B the more massive. Component A, SB2,,SB:4.77d, disproved; A is single. B resolved by speckle interferometry 1983.93, sep. 0.10".
HR 8321 12 BD+22 4472 207089 89972 3739 I 21 46 04.4 +22 56 56 5.29 K0IbHdel 0.5 e S:Strong He 10830 emission.
HR 8325 BD+24 4473 207134 89976 I 21 46 24.0 +25 33 48 6.28 K3III:
HR 8328 11 BD+02 4414 207203 127060 1574 21 47 14.0 +02 41 10 5.64 A1V
HR 8330 BD+16 4598 207223 107395 21 47 04.7 +17 11 39 6.21 F3V
HR 8341 BD+19 4793 207563 90027 3744 21 49 26.9 +20 27 45 6.29 B2V
HR 8343 14 BD+29 4525 207650 90040 1575 21 49 50.7 +30 10 27 5.04 A1V s G:Pleiades group.,SB:5.3047d, K 37.0k/s, V0 -23.9k/s, msin3i 0.0813, asini 2.29.
HR 8344 13 BD+16 4612 207652 107425 W 13891 21 50 08.7 +17 17 08 5.29 F2III-IV 2.0 0.2 D:5.5 F2, 7.5, 29.0y, a = 0.396"; previous orbits 37.594y, a = 0.433" and 27.508y, a = 0.387".,VAR:Delta Sct?
HR 8348 BD+19 4797 207840 107445 15383 21 51 34.2 +19 49 36 5.77 B8III 5.6 19.3 D:Both components optical.,S:Also classified B6Vp.
HR 8350 BD+20 5027 207932 90059 I HO Peg 21 52 18.2 +21 16 23 6.89 R M4III VAR:I, amp. 0.4B.
HR 8354 15 BD+28 4215 207978 90065 21 52 29.9 +28 47 36 5.53 F6IV-V vw S:Weak lines, no G-band. Metals indicate F4V; H and K, late F.
HR 8356 16 BD+25 4635 208057 90075 823 21 53 03.8 +25 55 30 5.08 B3Ve SB:17.79d?
HR 8358 BD+18 4879 208108 107474 21 53 37.4 +19 40 06 5.68 A0V s
HR 8359 BD+06 4919 208110 127141 21 53 57.8 +06 51 52 6.15 G0III s S:Also classified K0III.
HR 8364 BD+19 4814 208202 107489 15431 21 54 17.4 +19 43 06 6.39 K0III+F7V 2.1 22.3 D:AB CPM. Companion F7V.
HR 8372 BD+20 5046 208527 90112 1579 I 21 56 24.0 +21 14 23 6.40 K5V
HR 8373 17 BD+11 4696 208565 107528 3751 21 56 56.4 +12 04 35 5.54 A2Vnn
HR 8385 18 BD+06 4940 209008 127219 3759 22 00 07.9 +06 43 03 6.00 B3III
HR 8391 BD+32 4316 209149 71932 22 00 26.8 +33 00 22 6.46 F5III S:Also classified F6V, F7IV.
HR 8392 20 BD+12 4737 209166 107587 826 15543 22 01 05.4 +13 07 11 5.60 F4III 6.4 54.7
HR 8393 19 BD+07 4779 209167 127239 I 22 01 09.2 +08 15 26 5.65 gK5
HR 8397 BD+10 4676 209288 107599 14001 22 02 01.4 +10 58 26 6.37 B5IIIn
HR 8404 21 BD+10 4681 209459 107625 22 03 19.0 +11 23 11 5.80 B9.5V
HR 8412 BD+32 4329 209693 71998 15602 22 04 34.4 +32 56 31 6.38 G5Ia 4.8 21.4
HR 8413 ν 22 BD+04 4800 209747 127285 I 14020 22 05 40.8 +05 03 31 4.84 K4III
HR 8415 BD+25 4671 209761 90214 I 22 05 11.4 +26 40 26 5.78 K2III
HR 8419 23 BD+28 4284 209833 90217 3768 22 05 34.7 +28 57 50 5.70 B9Vn
HR 8430 ι 24 BD+24 4533 210027 90238 831 I W 14034 22 07 00.7 +25 20 42 3.76 F5V 7.4 103.7 D:Optical.,SB:10.2130d, K 49.1k/s, V0 -4.6k/s, asini 6.90.
HR 8435 BD+18 4930 210074 107675 22 07 28.6 +19 28 32 5.75 R dF2 G:Hyades group.
HR 8436 BD+17 4693 210090 107676 I 14039 22 07 30.0 +18 00 02 6.35 M1 VAR:6.3 - 7.7:v.
HR 8438 25 BD+21 4695 210129 90252 22 07 50.3 +21 42 10 5.78 B7Vne v M:Old disk population runaway star.,VAR:Emission variable in period over 50y.
HR 8441 BD+24 4540 210210 90259 22 08 17.2 +25 32 37 6.11 F1IV
HR 8449 π1 27 BD+32 4349 210354 72064 833 15672 22 09 13.6 +33 10 20 5.58 G8IIIb 5.8 70.2 D:Components B and C optical.
HR 8450 θ 26 BD+05 4961 210418 127340 834 14057 22 10 12.0 +06 11 52 3.53 A2Vp N:Baham; Biham.,S:Lambda Boo star, Mg 4481, Fe wk.,VAR:Delta Sct?
HR 8454 π2 29 BD+32 4352 210459 72077 835 22 09 59.2 +33 10 42 4.29 F5III G:Sirius group; UMa stream.,S:Shell star.
HR 8455 BD+18 4946 210460 107706 S 22 10 19.0 +19 37 01 6.18 G0V M:Possible nearby star on basis of spectroscopic parallax.
HR 8456 BD+13 4861 210461 107707 15690 22 10 22.2 +14 37 48 6.33 K0III 5.1 21.5
HR 8458 BD+10 4701 210502 107712 3773 I 22 10 37.4 +11 37 28 5.78 M1III
HR 8459 28 BD+20 5093 210516 90287 3772 22 10 30.2 +20 58 41 6.46 A3III
HR 8460 BD+29 4604 210594 72095 22 10 51.6 +30 33 11 6.32 A8IV
HR 8461 BD+15 4592 210702 107729 22 11 51.3 +16 02 26 5.95 K1III G:UMa stream.
HR 8466 BD+24 4548 210762 90317 I 22 12 08.0 +24 57 00 5.92 K0
HR 8475 BD+33 4456 210889 72132 3776 I 22 12 47.8 +34 36 17 5.33 K2-III-IIIb
HR 8482 BD+27 4280 211006 90337 22 13 38.6 +28 36 30 5.89 K2III
HR 8491 BD+07 4834 211287 127420 3780 22 15 59.8 +08 32 58 6.21 A1Vn
HR 8503 BD+27 4288 211432 90379 22 16 29.7 +27 48 15 6.37 G9III
HR 8513 30 BD+05 4998 211924 127453 15847 14122 22 20 27.6 +05 47 22 5.37 B5IV 5.9 14.8 D:AB CPM. B, 10.7v A7V at 6"; C, F6IV, optical.
HR 8514 BD+07 4853 211976 127460 22 20 55.8 +08 11 12 6.17 F6V
HR 8517 BD+26 4410 212047 90437 I 14127 22 21 00.1 +26 56 07 6.47 M4III
HR 8520 31 BD+11 4784 212076 107854 843 IN Peg 22 21 31.1 +12 12 19 5.01 B2IV-Ve v S:Shell star.,VAR:Amp. 0.43V. Emission var. period about 8y.
HR 8522 32 BD+27 4299 212097 90440 15863 22 21 19.3 +28 19 50 4.81 B9III 6.3 72.6
HR 8532 33 BD+20 5139 212395 90462 15896 22 23 39.6 +20 50 54 6.04 R F7V 2.2 78.4 D:AB binary. B, 9.2v at 2.5" in 1832; 0.296" by speckle interferometry on 1985.5.,DYN:0.025".
HR 8543 BD+17 4746 212670 107906 1586 22 25 40.7 +18 26 40 6.26 K0
HR 8548 34 BD+03 4705 212754 127529 15935 22 26 37.4 +04 23 37 5.75 F7V 6.5 3.3 D:AB binary. B is K4.,DYN:0.017".,G:Hyades moving group.
HR 8551 35 BD+03 4710 212943 127540 3796 I W 22 27 51.5 +04 41 44 4.79 K0III 4.9 181.5
HR 8555 BD+31 4701 212988 72366 I 22 27 46.2 +31 50 25 5.98 K2
HR 8562 36 BD+08 4874 213119 127544 1588 I 22 29 08.0 +09 07 44 5.58 K5IIIa
HR 8564 BD+26 4439 213179 90544 1589 22 29 10.2 +26 45 47 5.79 K2II
HR 8566 37 BD+03 4713 213235 127551 15988 22 29 58.0 +04 25 54 5.48 F2V+F2V 1.4 0.9 D:5.77 F5IV, 7.14 F7IV, 143.0y, a = 0.746" or 140.0y, a = 0.75". Combined mag., colors.,DYN:0.018".,S:Also classified A7m. K,H,met indicate A8,F1,F2, respectively.,SB:A4, F8, ADS 15988A, 372.4d, K 8.2k/s, V0 0.0k/s, asini 36.8. Poor phase distribution (orbit questioned) according,SB:to Morbey and Griffin (1987, ApJ, 317, 343).
HR 8574 38 BD+31 4708 213323 72406 1590 S 22 30 01.8 +32 34 21 5.65 B9.5V 0.2
HR 8584 BD+28 4389 213534 90568 GX Peg 22 31 34.2 +29 32 34 6.35 A5m S:Also classified A8V.,SB:2.3410d, K 84.9k/s, V0 +1.0k/s, asini 2.73. Apsidal period 260?y.,VAR:Delta Sct 6.30 - 6.32v, 0.056d.
HR 8586 39 BD+19 4949 213617 107986 3804 22 32 35.5 +20 13 48 6.42 F1V G:Hyades group.
HR 8587 BD+15 4670 213644 107989 3806 22 32 46.9 +15 51 48 6.32 K0
HR 8604 BD+34 4728 214200 72517 W 22 36 07.9 +35 34 38 6.10 K0 D:Probably single.
HR 8605 BD+10 4781 214203 108036 22 36 36.4 +11 41 49 6.40 A1III
HR 8608 BD+11 4838 214298 108043 I 22 37 04.7 +12 34 38 6.30 K5
HR 8618 40 BD+18 5014 214567 108064 W 22 38 52.6 +19 31 20 5.82 G8II 5.6 1.5
HR 8624 41 BD+18 5021 214698 108078 22 39 47.0 +19 40 52 6.21 R A2V
HR 8631 BD+13 4971 214850 108094 16173 22 40 52.7 +14 32 58 5.71 G4V 0.5 0.4 D:AB 6.26 G3V, 6.81 G8V, 20.93y, a = 0.30". Combined mag., colors. Perhaps invisible companion, period 15.8y. ADS 16173C,,D:11.6v at 72". Faint CPM, 14.9v at 4.5' N. prec.,DYN:0.027".
HR 8634 ζ 42 BD+10 4797 214923 108103 855 16182 22 41 27.7 +10 49 53 3.40 B8V 8.9 64.3 N:Homam; Homan; Humam; Al Hammam.
HR 8638 BD+30 4771 214979 72625 I 22 41 31.4 +30 57 57 6.34 R K5
HR 8641 ο 43 BD+28 4436 214994 90717 22 41 45.4 +29 18 27 4.79 A1IV G:In Ursa cluster?
HR 8642 BD+13 4974 214995 108109 22 41 57.4 +14 30 59 5.90 gK0
HR 8650 η 44 BD+29 4741 215182 90734 857 I 16211 14285 22 43 00.1 +30 13 17 2.94 G2II-III+F0V 5.1 90.4 D:A* 2.94 G2II-III, 2.23y, a = 0.022". Speckle interferometry measures range from unresolved to sep. 0.059". BC, 10.0,,D:10.0v sep. 0.2" at 90" from A, physical.,N:Matar.,SB:ADS 16211A, 818.0d, K 14.2k/s, V0 +4.3k/s, asini 158, vsini of G8 component 9k/s, F0 component =<50k/s.,VAR:ADS 16211A.
HR 8653 BD+10 4805 215243 108131 22 43 42.7 +10 56 21 6.51 G8IV S:Also classified F6Vn; HD, F5.
HR 8660 45 BD+18 5046 215510 108154 1596 22 45 28.2 +19 22 00 6.25 gG6
HR 8665 ξ 46 BD+11 4875 215648 108165 I 16261 22 46 41.6 +12 10 22 4.19 F6III-IV 7.5 145.0 D:AB binary. B 12v M1 at 12"; C, optical.,G:Wolf 630 group.
HR 8667 λ 47 BD+22 4709 215665 90775 859 I 22 46 31.9 +23 33 56 3.95 G8IIIa* S:G8IIIa CN1 Ba 0.3 H delta-1
HR 8681 BD+09 5111 216048 108204 22 49 32.3 +10 28 44 6.54 F0IV-V
HR 8684 μ 48 BD+23 4615 216131 90816 862 I 22 50 00.2 +24 36 06 3.48 G8+III
HR 8691 BD+18 5059 216201 108211 22 50 39.1 +19 08 27 6.40 R K0
HR 8697 σ 49 BD+09 5122 216385 127810 3828 22 52 24.1 +09 50 08 5.16 F7IV 8.4 248. D:CPM companion M4.
HR 8703 BD+16 4831 216489 108231 3829 IM Peg 22 53 02.3 +16 50 28 5.64 K1-2II-III e S:CaII emission.,SB:24.65d, K 33.2k/s, V0 -12.8k/s, asini 11.3. Close radio binary.,VAR:Amp. 0.16V. Out of phase with orbital period.
HR 8714 BD+16 4833 216672 108246 I HR Peg 22 54 35.7 +16 56 30 6.12 S4+/1+ VAR:Amp. 0.2:V, 50:d.
HR 8717 ρ 50 BD+08 4961 216735 127839 22 55 13.7 +08 48 57 4.90 A1V
HR 8724 BD+11 4904 216900 108275 16389 22 56 51.5 +11 50 54 6.51 A3V s 3.0 3.9
HR 8729 51 BD+19 5036 217014 90896 14374 22 57 27.9 +20 46 08 5.49 G2.5IVa S:Also classified G5V.
HR 8737 BD+08 4973 217166 127870 16417 14379 22 58 35.1 +09 21 25 6.43 G2V+G4V 0.2 0.2 D:AB 7.1 G2V, 7.3 G4V, 26.5y, a = 0.39".,DYN:0.034".,G:Zeta Her group.,VAR:Combined mag. ADS 16417AB varies slightly.
HR 8739 52 BD+10 4859 217232 108307 16428 22 59 11.8 +11 43 44 5.75 A8V+F6V 1.3 0.7 D:6.1 F0V, 7.4 F6V, 270.13y, a = 0.815". Combined mag., colors.,S:Primary variously classified A7V, A8V, F0V, or A8III.
HR 8753 BD+30 4859 217477 72924 16443 23 00 42.5 +31 04 59 6.60 B9IIIpMn 2.5 3.4 D:CPM.
HR 8765 BD+31 4829 217754 72949 23 02 33.1 +31 46 50 6.57 F2IV
HR 8775 β 53 BD+27 4480 217906 90981 870 I 16483 Bet Peg 23 03 46.5 +28 04 58 2.42 M2.5II-III e 7.0 253.1 N:SCHEAT; Sheat; Seat Alpheras; Menkib.,S:Ultraviolet FeII emission.,VAR:Lb 2.31 - 2.74V.
HR 8781 α 54 BD+14 4926 218045 108378 871 I 14417 23 04 45.7 +15 12 19 2.49 B9V N:MARKAB; Marchab.
HR 8784 BD+15 4760 218101 108383 23 05 06.3 +16 33 47 6.44 G8IV
HR 8788 BD+17 4866 218235 108400 23 06 18.2 +18 31 03 6.13 F6V s G:Hyades moving group.
HR 8792 BD+19 5058 218261 108402 23 06 31.9 +19 54 39 6.30 F7V G:Hyades group.
HR 8795 55 BD+08 4997 218329 127976 1603 I 14428 23 07 00.3 +09 24 34 4.52 M1IIIab
HR 8796 56 BD+24 4716 218356 91019 3848 I 14429 23 07 06.8 +25 28 06 4.76 G8Ib G:Wolf 630 group.,S:BaII star? Also classified K0IIp, BaII:. White dwarf companion.
HR 8798 BD+32 4587 218395 73010 16519 A 14430 23 07 27.7 +32 49 33 6.02 R A4Vn 1.5 8.4 D:Binary.,S:Metallic line star. K/H/met give A2/A3V/F0.,VAR:ADS 16519. Uncertain which component varies, if either.
HR 8799 BD+20 5278 218396 91022 3850 Var 23 07 28.7 +21 08 03 5.99 A5V SB:Possibility this is a metal-poor double star.,VAR:Possible delta Sct type. Amp. 0.08V.
HR 8815 57 BD+07 4981 218634 128001 I 16550 GZ Peg 23 09 31.5 +08 40 38 5.12 M4IIIS+A2V 5.5 32.9 SB:ADS 16550A companion 8v A3V unresolved by speckle interferometry. Primary over 5 solar masses; companion 2 solar,SB:masses; orbital period over 0.4yrs. vsini of M4 component =<50k/s, A2 component =<90:k/s.,VAR:ADS 16550A, Lb? 5.0 - 5.16V.
HR 8821 58 BD+09 5170 218700 128007 23 10 01.5 +09 49 19 5.39 B9III G:In Ursa cluster?
HR 8824 BD+16 4882 218792 108443 I 23 10 42.6 +17 35 40 5.71 K4III
HR 8826 59 BD+07 4991 218918 128022 1606 23 11 44.2 +08 43 12 5.16 A5Vn
HR 8827 60 BD+26 4580 218935 91080 W 23 11 49.2 +26 50 50 6.17 G8III-IV 3.3 231.5 G:Gamma Leo group.
HR 8831 BD+28 4548 219110 91095 23 13 04.0 +29 26 30 6.35 G8III
HR 8833 BD+10 4902 219139 108463 3858 16603 23 13 26.5 +11 03 54 5.82 G8III 3.9 33.3 C:Discordant UBV data: 5.820 and 5.579V, +1.008 and +0.989(B-V).,D:Probably optical.
HR 8838 BD+28 4555 219291 91111 W 23 14 21.7 +29 46 18 6.41 F6IV w 3.5 34.9
HR 8839 BD+23 4704 219310 91113 23 14 36.5 +24 06 11 6.36 R K2III
HR 8842 61 BD+27 4521 219477 91130 3861 23 15 46.3 +28 14 52 6.49 G5II-III
HR 8845 BD+23 4712 219487 91133 23 15 57.9 +24 46 16 6.60 F5V
HR 8873 BD+34 4899 219927 73171 23 19 27.4 +34 47 36 6.32 B8III
HR 8880 τ 62 BD+22 4810 220061 91186 880 Tau Peg 23 20 38.2 +23 44 25 4.60 A5Vp N:Salm; Kerb; Markab; El khereb.,S:Lambda Boo star, Mg 4481, met. wk.,VAR:Delta Sct 4.60 - 4.62V, 0.05433d, secondary 0.04895d, beat period 0.4943d.
HR 8882 63 BD+29 4908 220088 73187 I 23 20 49.6 +30 24 54 5.59 M0III
HR 8887 64 BD+31 4897 220222 73205 16702 23 21 54.9 +31 48 45 5.32 B6III 3.7 0.4
HR 8888 BD+25 4924 220242 91208 23 21 58.2 +26 36 32 6.62 F5V
HR 8891 65 BD+20 5317 220318 91220 3873 23 22 40.5 +20 49 43 6.29 B9.5V SB:22.635d, K 20.8k/s, V0 -9.8k/s, e 0.072, asini 6.5.
HR 8893 66 BD+11 4993 220363 108580 I 16715 23 23 04.6 +12 18 50 5.08 K3III 0.0 0.1 D:Interferometer double.
HR 8899 BD+31 4901 220460 73223 23 23 47.5 +32 31 53 6.69 F4V w SB:6.0499d, K 48.2k/s, V0 +12.6k/s, msin3i 0.300, asini 4.01. Rare example of short period binary with,SB:metal-deficient components.
HR 8903 67 BD+31 4904 220599 73241 1613 23 24 50.8 +32 23 06 5.57 B9III
HR 8905 υ 68 BD+22 4833 220657 91253 881 I 23 25 22.8 +23 24 15 4.40 F8III G:Hyades moving group.
HR 8915 69 BD+24 4778 220933 91278 HV Peg 23 27 40.4 +25 10 02 5.98 A0pHgMn G:Member of Pleiades group.,VAR:Amp. 0.012V, 6.97d.
HR 8922 BD+22 4844 221113 91295 23 29 05.6 +23 02 52 6.35 R G9III
HR 8923 70 BD+11 5009 221115 108638 885 I 23 29 09.3 +12 45 38 4.55 G7+III
HR 8933 BD+27 4568 221394 91321 Var 23 31 43.1 +28 24 13 6.41 A1pSrCr:Eu: VAR:Amp. 0.06V.
HR 8936 BD+34 4948 221491 73325 23 32 24.6 +34 57 09 6.65 B8V
HR 8940 71 BD+21 4952 221615 91340 3889 I HW Peg 23 33 28.1 +22 29 56 5.32 M5IIIa D:Spectrum binary unresolved by speckle interferometry.,VAR:7.0 - 7.30p.
HR 8942 BD+20 5352 221662 91349 I 23 33 55.5 +20 50 27 6.06 M3III
HR 8943 72 BD+30 4978 221673 73341 I 16836 14617 23 33 57.2 +31 19 31 4.98 K4IIIb 0.2 0.5 D:5.6 K4III, 5.7 K5III, 241.20y, a = 0.447".,DYN:0.005".,VAR:ADS 16836. Uncertain which component varies.
HR 8948 73 BD+32 4667 221758 73345 3891 23 34 38.2 +33 29 50 5.63 gK0
HR 8953 BD+23 4769 221905 91367 3894 I 23 35 55.9 +24 33 40 6.45 M1III
HR 8960 74 BD+16 4954 222098 108729 W 23 37 39.8 +16 49 32 6.26 A1V 4.5 98.3 SB:11.2298d, K 26.7k/s, V0 -27.4k/s, asini 4.12. RV of He 10830, same period.
HR 8963 75 BD+17 4952 222133 108732 3896 W KS Peg 23 37 56.8 +18 24 02 5.53 A1Vn 6.2 27.9 RV:SB 0.5021035d.,VAR:Ellipsoidal var, amp. 0.08B. Period consistent with SB.
HR 8970 BD+08 5095 222377 128309 23 39 55.1 +09 40 38 5.97 A2IVm
HR 8991 77 BD+09 5268 222764 108789 3902 I 14679 23 43 22.4 +10 19 53 5.06 M2III VAR:Amp. 0.05V.
HR 8997 78 BD+28 4627 222842 91457 I 16957 23 43 59.5 +29 21 42 4.93 K0III 3.1 0.9 DYN:0.010".
HR 9025 79 BD+28 4649 223461 91522 3913 23 49 39.4 +28 50 33 5.97 A2m
HR 9030 80 BD+08 5127 223637 128421 I HH Peg 23 51 21.2 +09 18 48 5.79 M3IIIa VAR:Lb? 5.74 - 6.0V.
HR 9035 BD+20 5386 223755 91548 I 23 52 23.4 +21 40 15 6.11 M2III
HR 9036 φ 81 BD+18 5231 223768 108878 898 I 14735 23 52 29.3 +19 07 13 5.08 M2.5IIIb
HR 9039 82 BD+10 5004 223781 108879 1625 HT Peg 23 52 37.1 +10 56 51 5.30 A4Vn VAR:Delta Sct, amp. 0.01V, 0.06d.
HR 9051 BD+25 5042 224128 91582 23 55 23.0 +25 57 18 6.54 R K5
HR 9055 BD+21 4999 224303 91595 1628 I 23 56 41.5 +22 38 53 6.15 M2III
HR 9064 ψ 84 BD+24 4865 224427 91611 1629 I S 14777 23 57 45.5 +25 08 29 4.66 M3III G:UMa stream.,VAR:4.63 - 4.69V.
HR 9078 BD+26 4727 224758 91648 W 00 00 23.9 +26 55 06 6.46 F7-8IV-V D:Probably single.
HR 9088 85 BD+26 4734 224930 91669 17175 14809 00 02 10.2 +27 04 55 5.75 G5VbFe-2 3.1 75.5 D:AB 5.84 G3V, 8.88 K6V, 26.386y, a = 0.803". A possible new companion found by speckle interferometry. Components C, D,D:probably optical. C is K7V.,DYN:0.081".,SB:ADS 17175AB, 26.27y D, K 5.1k/s, V0 -37.9k/s, asini 622.
HR 9109 BD+25 5068 225276 73731 I 42 00 04 56.0 +26 38 56 6.25 K4IIIb 4.5 17.5

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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