Kataloge

Auriga / 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 1501 BD+32 827 29867 57393 04 43 48.3 +32 51 55 6.45 R A8V
HR 1528 BD+32 840 30453 57444 S 04 49 19.0 +32 35 18 5.86 A8m SB:7.0507d, K 57.8k/s, V0 +20.3k/s, asini 5.60.
HR 1529 BD+31 816 30454 57441 2359 I 04 49 12.8 +31 26 14 5.58 K2III
HR 1535 BD+48 1162 30557 39799 2361 04 51 09.3 +48 44 27 5.66 G9III
HR 1550 BD+42 1081 30823 39826 04 52 47.8 +42 35 12 5.71 A3III
HR 1551 2 BD+36 952 30834 57475 I 04 52 38.0 +36 42 11 4.78 K2.5IIIbBa0.4 G:Sirius group; UMa stream.
HR 1558 BD+43 1116 31069 39851 04 54 51.3 +44 03 39 6.08 A0V
HR 1573 BD+35 930 31327 57511 04 56 19.9 +36 10 08 6.07 B2Ib G:Aur OB1.
HR 1577 ι 3 BD+32 855 31398 57522 181 I 1778 04 56 59.6 +33 09 58 2.69 K3II N:Hassaleh in Becvar.,VAR:4.0 - 4.15p.
HR 1592 ω 4 BD+37 1005 31647 57548 3572 04 59 15.4 +37 53 25 4.94 A1V 2.8 5.1 D:Binary.,DYN:0.021".,G:Pleiades group.
HR 1599 5 BD+39 1133 31761 57559 3589 05 00 18.3 +39 23 41 5.95 F5V 3.4 3.7 DYN:0.037".
HR 1602 6 BD+39 1134 31780 57560 I 05 00 23.2 +39 39 18 6.58 R K4I
HR 1605 ε 7 BD+43 1166 31964 39955 183 I 3605 Eps Aur 05 01 58.1 +43 49 24 2.99 F0Iae+B v 6.2 207.6 D:ADS 3605A. A* 2.98 var. A8Iap. Five visual and one astrometric components. AB visual binary, B, 14v at 29"; C,,D:11.26V, +1.83(B-V), +1.31(U-B), at 43"; D, 12.0v at 46".,N:Al Anz; Almaaz.,S:Shell star. Also classified A8Ia-F2epIa + B.,SB:ADS 3605A, 9890d, K 15.0k/s, V0 -1.4k/s, msin3i 16.8, asini 2000. Unresolved by speckle interferometry.,VAR:ADS 3605A, EA 2.94 - 3.83V, 9892d. Spectrum var. even outside eclipse. RV and light fluctuations about 110d.
HR 1612 ζ 8 BD+40 1142 32068 39966 1137 I Zet Aur 05 02 28.7 +41 04 33 3.75 K4II+B8V N:Haedi; Haedus; Hoedus I. With HR 1641, one of the "kids"; Sadatoni; Saclateni.,S:Also classified K5II + B5V.,SB:972.162d, K 24.6k/s, V0 +12.9k/s, msin3i 7.54, asini 300. Unresolved by speckle interferometry . SKYLAB,SB:indicates cool star with hot companion.,VAR:EA 3.70 - 3.97V, 972.164d, i 90d. Variable duration of min. Amp. depends on wavelength, 0.55B, 1.97U. K component,VAR:amp. 0.05V.
HR 1615 BD+41 1044 32188 39979 1810 05 03 18.6 +41 26 30 6.14 A2IIIShell? S:H alpha, beta and gamma have absorption cores. TiII and FeII stronger than normal; MgII, SiII strong. Shell doubtful.
HR 1626 BD+30 772 32406 57610 05 04 14.5 +30 29 41 6.14 K0II-III
HR 1627 BD+32 879 32428 57614 05 04 36.9 +32 19 13 6.62 A4m S:Also classified A8.5Vm:
HR 1637 9 BD+51 1024 32537 25019 3675 05 06 40.6 +51 35 52 5.00 F0V 4.4 90.1 D:A,B,C, CPM; D, optical; E, 12.3v at 132" from A.,SB:ADS 3675A, 391.7d, K 5.8k/s, V0 -7.4k/s, asini 29.0.
HR 1639 BD+35 973 32608 57629 2379 05 06 00.9 +35 56 11 6.52 A5V
HR 1641 η 10 BD+41 1058 32630 40026 185 1822 05 06 30.9 +41 14 04 3.17 B3V G:Cas-Tau OB1; member of Pleiades group.,N:Hoedus II. One of the kids, with HR 1612.,RV:Doubtful var., 24d period not confirmed.,VAR:Beta C?
HR 1644 BD+42 1170 32655 40029 05 06 49.6 +43 10 29 6.20 F2IIp:
HR 1668 BD+46 970 33167 40077 05 10 42.9 +46 57 44 5.68 F5V G:Hyades moving group.
HR 1669 BD+37 1067 33203 57704 I 3734 05 10 18.9 +37 18 07 6.02 K3:+B2II: 0.1 1.5 D:AB, CPM.
HR 1689 μ 11 BD+38 1063 33641 57755 192 05 13 25.7 +38 29 04 4.86 A4Vm
HR 1692 BD+53 872 33654 25087 2393 05 14 44.3 +53 12 50 6.20 A0V
HR 1706 14 BD+32 922 33959 57799 3824 A KW Aur 05 15 24.4 +32 41 16 5.02 A9IVDel Del 2.9 14.3 D:AC binary. B, 11v F4V at 13" optical.,G:Possible new Eggen group with HR 63, q.v.,SB:ADS 3824A, 3.788506d, K 23.0k/s, V0 -9.8k/s, asini 1.20.,VAR:Delta Sct 4.94 - 5.10V, 0.088088d. Form of light curve varies. Also nonradial pulsations of 0.096533 and 0.088243d.
HR 1707 BD+53 882 34019 25112 I 3845 R Aur 05 17 17.8 +53 35 10 6.50 M7IIIe 2.1 46.4 D:Binary. Component B, 9.50V, +0.47(B-V), +0.09(U-B), F4IV.,S:Probable SiO maser emission.,VAR:ADS 3845A, M 6.7 - 13.7v, 457.64d, period changes; 10.18 - 13.12V, -0.06 to -0.43(U-B). Cycle of 64.5d also possible.
HR 1708 α 13 BD+45 1077 34029 40186 193 I 3841 1897 05 16 41.4 +45 59 53 0.08 G5IIIe+G0III v 0.5 0.0 D:AP 0.6 G5III, 1.1 G0III, sep. 0.04", 0.285y, a = 0.054", masses 2.67 and 2.55 solar. Combined mag., colors. Capella is,D:first star for which an orbit was determined from interferometer measures, by Anderson at Mt. Wilson in 1920. Speckle,D:sep. 0.040" 1981.24 and 1981.68; 0.055" 1982.16. CPM with component H, a close binary, 10.0 dM1, 13.7 dM5 sep. 2" at,D:723" from A, probably physical with A. Other components all faint and distant from A.,DYN:0.058".,G:Hyades group.,N:CAPELLA; Alhajoth.,R:Diam. component A = 0.0052", component B = 0.0040".,S:Chromospheric He 10830 double. Balloon-borne spectrometer revealed pronounced emission of MgII. Soft X-ray emission.,S:Lithium content of the F-type component is 15 times that of the G component. Also classified G6III+F9III.,SB:104.0204d, K 26.1k/s, V0 +29.5k/s, asini 37.3.,VAR:Amp. 0.03V. Variable helium and X-ray emission.
HR 1712 BD+34 980 34078 57816 3843 AE Aur 05 16 18.2 +34 18 43 5.96 O9.5V e 3.3 8.4 D:Component B doubtful, possibly the nebula. C 10.7V at 30".,G:Runaway star from Ori OB1 association. Moving at 128k/s in opposite direction from Mu Col = HR 1996. See HR 938.,G:Exciting star of HII region S229; associated with nebula IC 405. S229 superimposed on S230. In reflection nebula. The,G:best example of nebulosity in which the gas and dust are differently distributed.,S:Central Balmer emission in blue-violet only.,VAR:ADS 3843A, Ina 5.78 - 6.08V. Possibly a SN 2.5 million yrs. ago.
HR 1722 BD+42 1239 34269 40214 I PU Aur 05 18 15.9 +42 47 32 5.48 M4III VAR:Lb?, amp. 0.10V.
HR 1725 BD+40 1240 34332 40224 05 18 40.4 +40 27 54 6.18 K0
HR 1726 16 BD+33 1000 34334 57853 I 3872 1909 05 18 10.7 +33 22 18 4.54 K2.5IIIbFe-1 5.8 4.2 D:CPM.,S:Also classified K2.5IIIb CN-0.5.,SB:ADS 3872A, 434.8d, K 14.8k/s, V0 -27.5k/s, asini 88.0.,VAR:ADS 3872A, E?
HR 1728 17 BD+33 1002 34364 57858 AR Aur 05 18 18.9 +33 46 02 6.14 B9.5V D:Possible CPM with HR 1732.,G:Aur OB1. Concentration of hydrogen emission in direction of this association.,S:Also classified ApHgMn + B9V.,SB:4.1346d, K 107.2k/s, V0 +25.1k/s, msin3i 2.48, asini 6.09; vsini of secondary 62k/s.,VAR:EA 6.15 - 6.82V, 6.05 - 6.72B, A0 + A0, 4.134695d, changing period.
HR 1729 λ 15 BD+39 1248 34411 40233 1145 3886 05 19 08.5 +40 05 57 4.71 G1.5IV-VFe-1 4.9 146.6 D:B, 13.4v at 29". C, 12.1v at 42" and D, optical.,G:Epsilon Ind group.
HR 1732 BD+33 1008 34452 57884 IQ Aur 05 19 00.0 +33 44 54 5.41 A0pSi v D:Possible CPM with HR 1728.,S:Magnetic star showing chlorine. Silicon star. Helium and neon deficient. Bluest known peculiar A-star: color,S:characteristic of about B4V. Classified A0p because He weak, but in other respects the color is more indicative of the,S:temperature than the spectral class of Ap stars. One of the hottest Ap stars known, about 17000K.,SB:Double lines.,VAR:Alpha CV 5.35 - 5.41V, 2.4660d. Spectrum var. same period.
HR 1733 BD+44 1170 34498 40242 05 20 02.3 +44 25 32 6.62 R K0
HR 1734 18 BD+33 1010 34499 57893 3893 05 19 23.6 +33 59 08 6.49 A7V 5.3 3.8
HR 1736 BD+46 998 34533 40251 3903 05 20 39.3 +46 57 50 6.54 GIII+A2V 2.9 23.2 D:Fixed. Companion spectral class A.
HR 1738 BD+40 1253 34557 40248 05 20 14.8 +41 05 10 5.52 A3V
HR 1740 19 BD+33 1013 34578 57906 2399 1925 05 20 00.9 +33 57 29 5.03 A5II
HR 1749 ρ 20 BD+41 1162 34759 40269 2400 05 21 48.4 +41 48 16 5.23 B3V G:Cas-Tau OB1.,SB:35.5d, K 28k/s, V0 +19k/s, asini 13.7.
HR 1752 BD+29 869 34790 77124 05 21 12.7 +29 34 12 5.76 R A1V s 0.4 0.0 SB:6.2, 6.6v, sep. 0.0005", 2.1517d, K 113.3k/s, V0 -19.7k/s, msin3i 1.71, asini 3.35; vsini both components 53k/s.
HR 1760 BD+40 1268 34904 40290 05 22 50.3 +41 01 46 5.54 A3V
HR 1768 22 BD+28 788 35076 77139 05 23 22.9 +28 56 12 6.46 B9V s
HR 1773 σ 21 BD+37 1175 35186 57981 I 3984 05 24 39.2 +37 23 08 4.99 K4III 7.0 8.7 D:AB fixed.
HR 1775 BD+31 954 35238 57987 05 24 38.3 +31 13 26 6.28 K1III
HR 1776 BD+31 955 35239 57988 05 24 38.5 +31 08 35 5.94 B9III
HR 1779 BD+34 1031 35295 57999 4000 A 05 25 13.0 +34 51 19 6.55 K1pIII-IV+F6V 1.8 31.2 D:CPM. Companion F6V.,S:Component A has abnormally strong CN. Lambda 4150 star.
HR 1794 BD+35 1102 35519 58029 2408 I 05 26 54.3 +35 27 26 6.15 K2 G:Open cluster NGC 1907 #1.
HR 1795 BD+34 1040 35520 58028 05 26 48.9 +34 23 30 5.94 A0III S:Also classified A1p.
HR 1796 BD+33 1045 35521 58030 05 26 51.3 +33 15 46 6.15 K0
HR 1804 BD+30 898 35600 58040 05 27 08.3 +30 12 31 5.74 B9Ib G:Aur OB1. Concentration of hydrogen emission in direction of this association.
HR 1805 φ 24 BD+34 1048 35620 58051 I W 05 27 38.9 +34 28 33 5.07 K3IIICN+2 3.2 206.8 G:Hyades group.
HR 1822 BD+29 909 35984 77205 05 29 40.6 +29 11 11 6.24 F6III
HR 1824 BD+41 1206 36040 40387 2412 05 30 48.6 +41 27 43 6.00 K0IIIp S:Lambda 4150 star.
HR 1825 BD+39 1322 36041 58129 W 05 30 45.1 +39 49 33 6.37 G9III 1.3 75.4 D:Companion 7.62V, +0.94(B-V), +0.69(U-B), G8III.
HR 1843 χ 25 BD+32 1024 36371 58164 1151 05 32 43.7 +32 11 31 4.76 B5Iab G:Aur OB1. Concentration of hydrogen emission in direction of this association.,SB:655.16d, K 20.5k/s, V0 -0.2k/s, asini 182.
HR 1846 BD+41 1218 36404 40426 05 33 28.7 +42 06 32 6.55 B9IIIp:Hg:
HR 1850 BD+32 1028 36484 58179 05 33 27.5 +32 48 04 6.48 A2m
HR 1854 BD+34 1083 36499 58182 05 33 38.0 +34 43 33 6.27 A3IV
HR 1866 BD+54 914 36678 25276 2416 I 05 36 35.2 +54 25 44 5.73 M0III
HR 1869 BD+47 1178 36719 40466 2417 05 36 15.9 +47 42 55 6.11 dF0
HR 1884 BD+40 1346 36891 40481 05 36 52.4 +40 10 56 6.09 G3Ib+F
HR 1904 BD+33 1102 37138 58263 05 37 45.7 +33 33 33 6.33 K0
HR 1914 26 BD+30 963 37269 58280 4229 2485 05 38 38.1 +30 29 33 5.40 F9III+B9.5V 0.3 0.2 D:AB 6.0 G5III, 6.3 A2V, 53.2y, a = 0.135". Combined, mag., colors. C, 8.57V, +0.28(B-V), +0.09(U-B), F0V at 12",,D:physical; D, 11.5v at 33". Resolved by speckle interferometry 1983.93, sep. 0.12".
HR 1924 BD+29 947 37367 77354 05 39 18.4 +29 12 55 5.96 B2IV-V 2.0 0.0 G:Cas-Tau OB1.,SB:6.2, 8.2, sep. 0.00001", about 6.5d, K 9k/s.
HR 1925 BD+53 934 37394 25319 W 05 41 20.3 +53 28 52 6.23 K1V 2.8 688.0 D:Component B, 9.9v M1 at 99", is BD +53d935, CPM. Component D is F5. Other companions 12.4 and 12.8v.
HR 1938 BD+31 1048 37519 58319 2425 2537 05 40 35.9 +31 21 29 6.04 B9.5III-IVp:
HR 1939 BD+31 1049 37536 58322 I NO Aur 05 40 42.1 +31 55 15 6.11 M2IIIS G:Aur OB1.,VAR:Lc 6.13 - 6.30V.
HR 1945 BD+29 953 37646 77393 4262 A 05 41 21.0 +29 29 15 6.43 B8IV 0.4 26.1 D:CPM, B is 7.18V, -0.04(B-V), -0.14(U-B), B9.5V, vsini 120k/s.,SB:ADS 4254A.
HR 1971 ο 27 BD+49 1398 38104 40583 216 05 45 54.0 +49 49 35 5.47 A2VpCr G:UMa stream.
HR 1974 BD+40 1403 38189 40584 05 45 49.5 +40 30 26 6.58 A3Del Del
HR 1979 BD+42 1396 38358 40609 2431 05 47 14.7 +42 31 36 6.29 K0
HR 1995 τ 29 BD+39 1418 38656 58465 I 4398 05 49 10.5 +39 10 52 4.52 G8IIIFe-1 6.1 49.6 G:Ursa cluster? UMa stream.
HR 2003 BD+51 1117 38765 25411 2437 05 50 56.4 +51 30 53 6.29 K1III
HR 2011 υ 31 BD+37 1336 38944 58496 2440 I 2661 05 51 02.4 +37 18 20 4.74 M0+III-IIIbFe-0.5 VAR:Amp. 0.1V. Cycles 35-36d in 1970-1 not confirmed in other seasons.
HR 2012 ν 32 BD+39 1429 39003 58502 221 I 4440 05 51 29.4 +39 08 55 3.97 G9.5III* 7.3 54.6 D:Companion optical.,S:G9.5III CN 0.5 Fe 1 Ba 0.2:
HR 2018 BD+32 1109 39045 58504 I 4443 Var 05 51 25.7 +32 07 30 6.25 M3III v 5.9 15.2 M:High space velocity.,S:Spectrum may be variable.,VAR:Amp. 0.10V.
HR 2025 BD+39 1435 39182 58524 05 52 39.5 +39 34 28 6.45 R A2V
HR 2028 BD+33 1179 39225 58528 2443 I 2681 05 52 40.1 +33 55 03 5.98 M1.5II-III M:High space velocity.
HR 2029 ξ 30 BD+55 1027 39283 25450 1157 05 54 50.8 +55 42 25 4.99 A2V G:Sirius group?,N:Flamsteed also called this star 32 Cam = 30 Aur.,R:Radius relative to Sun = 2.6.,S:Lambda Boo type.
HR 2045 BD+51 1128 39551 25467 05 56 14.4 +51 48 14 6.49 R A5V
HR 2046 BD+31 1139 39586 58569 05 54 59.0 +31 42 06 5.90 A5IV
HR 2054 BD+49 1423 39743 40720 05 57 04.9 +49 01 46 6.47 G8III
HR 2066 BD+28 952 39866 77744 05 56 33.8 +28 56 32 6.32 A2II
HR 2077 δ 33 BD+54 970 40035 25502 225 I W 05 59 31.6 +54 17 05 3.72 K0-III 5.8 115.4
HR 2079 BD+55 1036 40062 25504 05 59 45.7 +55 19 15 6.44 A5m
HR 2080 BD+54 971 40083 25505 05 59 48.1 +54 32 50 6.14 K2III
HR 2081 BD+49 1428 40084 40743 05 59 21.8 +49 55 28 5.89 G5III SB:219.13d, K1 32.2k/s, K2 33.23k/s, V0 -4.09k/s, a1sini 97.1, a2sini 100.1.
HR 2088 β 34 BD+44 1328 40183 40750 227 I 4556 Bet Aur 05 59 31.7 +44 56 51 1.90 A2IV 8.9 184.6 D:AB binary. C, 14.1v at 13".,G:In Ursa cluster; Sirius group; UMa stream; UMa cluster.,N:Menkalinan; Menkalina.,R:Radius relative to Sun = 3.0.,SB:ADS 4556A, 3.9600d, K 107.5k/s, V0 -17.1k/s, msin3i 2.20, asini 5.85. Masses 2.33, 2.25 solar. Rotational,SB:velocities both components <30k/s. Second SB ever discovered, by Antonia Maury, 1889.,VAR:ADS 4556A, EA 1.89 - 1.98V, 1.93 - 2.02B, A2+A2, 3.9600421d, i 78.5d.
HR 2091 π 35 BD+45 1217 40239 40756 I Pi Aur 05 59 56.1 +45 56 13 4.26 M3II e C:Large infrared excess.,M:Radio star.,S:Ultraviolet FeII emission.,VAR:Lc 4.24 - 4.34V. Radio emission at 2.85cm indicates mass loss.
HR 2095 θ 37 BD+37 1380 40312 58636 I 4566 The Aur 05 59 43.3 +37 12 45 2.62 A0pSi 4.5 3.5 D:AB binary , combined mag., colors. B is 7.2v G2V. C, 11v at 49" optical.,DYN:0.032".,R:Radius 3.3 solar.,VAR:ADS 4566B. Alpha CV 2.62 - 2.70V. Amp. 0.43m at 1400A, 1.3735d. Magnetic field varies 3.618d.
HR 2096 BD+44 1332 40325 40769 4576 06 00 19.0 +44 35 31 6.22 K2III+K0III 4.0 34.2 D:AB probably binary. B, 11v at 2". Component C, K0III, optical.
HR 2101 36 BD+47 1227 40394 40778 06 00 58.6 +47 54 07 5.73 B9.5pSiFe
HR 2105 BD+48 1333 40486 40789 2458 I 06 01 43.1 +48 57 34 5.96 K0
HR 2110 BD+31 1164 40588 58657 06 01 10.2 +31 02 05 5.98 R A2V
HR 2112 BD+49 1441 40626 40801 06 02 48.7 +49 54 20 6.05 B9.5IV
HR 2115 BD+43 1421 40722 40808 06 02 53.6 +43 22 43 6.42 R K0
HR 2119 38 BD+42 1473 40801 40818 2461 06 03 18.0 +42 54 42 6.10 K0II G:Sigma Pup group.
HR 2122 BD+32 1166 40832 58688 06 02 55.1 +32 38 09 6.24 F4V
HR 2123 BD+51 1146 40873 25548 2463 4633 2804 06 04 29.1 +51 34 24 6.45 A7III 2.8 39.0 D:BC, 9.0, 10.0v, sep. 0.6", CPM with A.,VAR:Delta Sct?
HR 2132 39 BD+42 1477 41074 40840 2812 06 05 03.4 +42 58 54 5.87 F3V G:Hyades group.
HR 2137 BD+37 1405 41162 58716 4649 06 05 02.6 +37 57 51 6.34 K0III+A2 5.6 17.9 D:Confusion as to whether B or C is the brighter, B at 18", C at 84" from A.
HR 2139 BD+33 1236 41269 58727 06 05 34.0 +33 35 57 6.23 B9pSi
HR 2141 BD+35 1334 41330 58739 W 06 06 08.5 +35 23 15 6.12 G0V 3.4 122.0
HR 2143 40 BD+38 1377 41357 58749 2465 Var? 06 06 35.1 +38 28 58 5.36 A4m SB:28.28d, K 51.4k/s, V0 +16.9k/s, msin3i 1.35, asini 16.6.,VAR:Suspected of 0.01m variability.
HR 2146 BD+29 1112 41429 77958 I 4673 06 06 22.5 +29 30 45 6.08 M3II+F7V 5.0 10.0 D:CPM. Companion 10.72V, +0.90(B-V), +0.25(U-B), F7V.
HR 2147 BD+41 1357 41467 40868 06 07 26.9 +41 51 15 6.12 K0III
HR 2153 BD+41 1365 41636 40881 06 08 23.0 +41 03 20 6.36 G9III
HR 2172 BD+52 1041 42083 25613 06 11 46.0 +52 38 50 6.30 A5IIIm SB:106d, K 40.5k/s, V0 +13.5k/s, msin3i 1.55, asini 45.8; vsini both components 30k/s. Unresolved by speckle,SB:interferometry.
HR 2175 41 BD+48 1352 42126 40924 4773 B 06 11 36.5 +48 42 47 6.82 H A8V 0.8 7.7 D:Binary with HR 2176.,G:Hyades group.
HR 2176 41 BD+48 1352 42127 40925 4773 A 06 11 36.6 +48 42 40 6.09 H A3V 0.8 7.7 D:Binary with HR 2175.,G:Hyades group.
HR 2188 BD+51 1163 42466 25630 06 13 45.3 +51 10 21 6.04 K1III
HR 2189 BD+32 1217 42471 58852 2470 I 06 12 20.1 +32 41 36 5.78 M2IIIa
HR 2217 BD+36 1388 43017 58905 1167 4849 A 06 15 39.0 +36 08 55 6.92 F4IV 0.6 11.3 D:AB CPM. B is dF0; C 12.3v at 202" optical. D, 11.5v at 120" from A.
HR 2219 κ 44 BD+29 1154 43039 78143 1168 I 2877 06 15 22.7 +29 29 53 4.35 G8.5IIIb
HR 2228 42 BD+46 1122 43244 40999 06 17 34.7 +46 25 27 6.52 F0V G:UMa stream.
HR 2239 43 BD+46 1124 43380 41010 06 18 16.9 +46 21 38 6.38 K2III G:Eta Cep group.
HR 2264 45 BD+53 1008 43905 25681 2484 06 21 46.1 +53 27 08 5.36 F5III SB:6.5013d, K 31.7k/s, V0 -1.5k/s, asini 2.83.
HR 2272 BD+29 1190 44092 78259 06 21 12.1 +29 32 28 6.43 A1V s
HR 2289 ψ1 46 BD+49 1488 44537 41076 242 I Psi1 Aur 06 24 53.9 +49 17 17 4.91 K5-M0Iab-Ib VAR:Lc? 4.75 - 5.70V, 6.6 - 7.2p.
HR 2297 BD+29 1213 44766 78333 06 24 52.6 +29 42 26 6.71 B8IIIn
HR 2314 BD+47 1299 45105 41109 06 27 51.1 +47 24 19 6.56 A0V
HR 2319 BD+32 1300 45192 59096 06 27 35.5 +32 33 47 6.43 K0
HR 2332 48 BD+30 1238 45412 59128 RT Aur 06 28 34.1 +30 29 35 5.55 F8Ib v S:Also classified F4Ib-G1Ib.,VAR:CDelta 5.02 - 5.82V. Per. changing, 3.728365 before 1950, 3.728115 since. CaII emission on rising branch of light,VAR:curve. Blue companion suspected.
HR 2338 47 BD+46 1149 45466 41130 2496 I 06 30 03.0 +46 41 08 5.90 gK4
HR 2372 BD+32 1324 46052 59194 2500 WW Aur 06 32 27.2 +32 27 17 5.87 A3m+A3m: S:Also classified A3m: + A3m:,SB:2.5250d, K 115.6k/s, V0 -8.7k/s, msin3i 1.98, asini 4.01. Masses 1.92, 1.90 solar. vsini same for both,SB:components 35k/s.,VAR:EA 5.79 - 6.54V, 2.52501922d. Per. changes. Rot. line apsides per. about 40,000d.
HR 2383 BD+33 1356 46251 59222 06 33 42.7 +33 01 27 6.42 R A3V
HR 2398 49 BD+28 1168 46553 78524 2504 3032 06 35 12.1 +28 01 20 5.27 A0Vnn
HR 2405 BD+38 1539 46687 59280 I W UU Aur 06 36 32.9 +38 26 43 5.29 C5II 5.6 17.9 S:Infrared spectra show CO, CN and C2 molecules.,VAR:SRb 7.83 - 10.00B, 8.2 - 10.0p, 234d. Mean mag. varies in per. about 3500d.
HR 2419 51 BD+39 1690 47070 59316 250 I 06 38 39.5 +39 23 27 5.69 K5III G:Hyades group.
HR 2420 ψ3 52 BD+40 1665 47100 59319 06 38 49.2 +39 54 09 5.20 B8III
HR 2425 53 BD+29 1293 47152 78571 D 06 38 23.0 +28 59 03 5.79 B9npEu 0.0 0.1 D:Discovered by both occultation and speckle interferometry 1978, sep. 0.075"; 1983.93, sep. 0.13".,S:Spectra show Hg 4077; Eu, Cr enhanced. Overabundant elements are V by factor of 300; Sr by 1500; Y by 100 and rare,S:earths by hundreds of thousands.
HR 2427 ψ2 50 BD+42 1585 47174 41239 I W 06 39 19.9 +42 29 20 4.79 K3III 5.5 52.1
HR 2434 BD+44 1506 47270 41245 06 39 58.0 +44 00 50 6.41 R K1III
HR 2438 54 BD+28 1196 47395 78593 5289 3065 06 39 33.1 +28 15 47 6.03 B7III 1.6 0.8
HR 2452 BD+36 1482 47703 59365 2516 06 41 37.7 +35 55 55 6.46 F8III
HR 2459 ψ4 55 BD+44 1518 47914 41288 2517 I 06 43 05.0 +44 31 28 5.02 K5III
HR 2464 BD+37 1567 48073 59406 06 43 13.8 +37 08 49 6.19 K0
HR 2471 BD+36 1494 48272 59425 06 44 12.6 +36 06 35 6.31 R A2V
HR 2483 ψ5 56 BD+43 1595 48682 41330 255 5425 06 46 44.3 +43 34 39 5.25 G0V 3.4 36.2 D:Companion orange, optical.
HR 2487 ψ6 57 BD+48 1436 48781 41346 1176 I 06 47 39.6 +48 47 22 5.22 K0III
HR 2516 ψ7 58 BD+41 1536 49520 41380 2527 I W 06 50 45.9 +41 46 53 5.02 K3III 5.0 40.9 G:61 Cyg group.
HR 2532 BD+45 1359 49949 41406 06 53 07.6 +44 50 22 6.26 A8Vn
HR 2539 59 BD+39 1771 50018 59571 5534 OX Aur 06 53 01.5 +38 52 09 6.12 F2VDel Del v 3.9 22.3 D:AB fixed.,M:Space motion almost identical to that of the Sun.,S:Also classified A7n-F3IV.,VAR:Delta Sct 5.94 - 6.14V, primary period 0.115442, secondary 0.154412d.
HR 2541 60 BD+38 1636 50037 59576 S 06 53 13.4 +38 26 17 6.30 dF5 N:Sometimes this star, sometimes HR 2547 have been called Psi8 Aur. To avoid future confusion this designation,N:is abandoned for both.
HR 2542 BD+35 1511 50056 59574 I 3250 06 53 03.4 +35 47 19 6.01 K3III:
HR 2547 ψ8 61 BD+38 1638 50204 59589 06 53 57.0 +38 30 18 6.48 B9.5pSi N:See note for HR 2541.,S:Hg, Mn.
HR 2556 BD+46 1202 50384 41426 06 55 15.2 +45 49 35 6.34 K0III-IV G:Hyades group.
HR 2557 BD+44 1551 50420 41429 V352 Aur 06 55 14.7 +43 54 36 6.13 A9III VAR:Delta Sct 6.037 - 6.054y. About 4 hrs. One of most luminous Delta Sct stars: abs. mag. about 0.0V.
HR 2568 ψ9 BD+46 1203 50658 41446 Var? 06 56 32.3 +46 16 27 5.87 B8IIIe S:Shell star.,VAR:Emission var. about 16 yrs.
HR 2573 BD+46 1205 50763 41450 06 56 56.0 +46 42 18 5.86 gK0
HR 2600 62 BD+38 1656 51440 59658 2538 I 06 59 02.8 +38 03 08 6.00 K2III
HR 2675 BD+37 1660 53925 59812 07 08 36.3 +37 26 42 6.16 K1III
HR 2696 63 BD+39 1882 54716 59866 274 I 07 11 39.3 +39 19 14 4.90 K4III-IIIa
HR 2753 64 BD+41 1630 56221 41679 276 07 18 02.2 +40 53 00 5.78 A5Vn G:In Ursa cluster?
HR 2775 BD+42 1699 56941 41705 07 21 03.1 +42 39 20 6.35 K0
HR 2792 BD+39 1927 57263 60012 07 22 13.4 +38 59 46 6.40 K0
HR 2793 65 BD+37 1707 57264 60010 2568 I 6009 07 22 02.6 +36 45 38 5.13 K0III 5.5 11.4 D:AB CPM. C, 12.7v at 42" optical.
HR 2805 66 BD+40 1852 57669 41738 1191 I 07 24 08.5 +40 40 20 5.19 K1+IIIaCN1

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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