Catalogues

Hercules / 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 5914 χ 1 BD+42 2648 142373 45772 1416 15 52 40.5 +42 27 06 4.62 F8VFe-2Hdel -1 S:Lithium to hydrogen ratio about 12 times solar. Low metal content.,VAR:Variable intrinsic polarization observed Aug. 1974.
HR 5932 2 BD+43 2542 142780 45788 I 7335 15 54 37.9 +43 08 19 5.37 M3IIIBa0.3
HR 5938 4 BD+42 2652 142926 45790 Var? 15 55 30.6 +42 33 58 5.75 B9pe v S:Shell star. Also classified B8V.,SB:46.0227d, K 12.0k/s, V0 -19.3k/s, asini 7.17. RV period constant over 40 yrs. Shell-line RV also 46.023d.,VAR:Spectrum var. Balmer emission and metallic absorption vary in period about 30 yrs; H alpha profile varies in period,VAR:of =<1 min. A potassium flare observed June 21, 1965. Probable mass-transfer between components.
HR 5950 BD+40 2948 143209 64988 15 57 29.9 +39 41 43 6.31 K0 G:Probable Hyades group.
HR 5964 BD+50 2239 143584 29737 3260 15 59 04.4 +49 52 52 6.05 F0IV
HR 5966 5 BD+18 3101 143666 101879 3263 I 16 01 14.3 +17 49 06 5.12 G8IIIbFe-0.5
HR 5982 υ 6 BD+46 2142 144206 45865 3271 16 02 47.9 +46 02 12 4.76 B9III S:HgMn star.
HR 6008 κ 7 BD+17 2964 145001 101951 1421 9933 A 7471 16 08 04.5 +17 02 49 5.00 G8III 1.2 28.1 D:Optical pair with HR 6009.,N:Marfik; Marsik; Mirfak; Marfak.,S:Also classified G8II, G7III.
HR 6009 κ 7 BD+17 2965 145000 101952 I 9938 B 16 08 04.9 +17 03 16 6.25 K1III 1.2 28.1 D:Optical pair with HR 6008.,S:Also classified K0IV, K2II and K2III.
HR 6013 8 BD+17 2967 145122 101962 7477 16 08 46.6 +17 12 21 6.14 A0Vnn
HR 6023 φ 11 BD+45 2376 145389 45911 601 7490 16 08 46.2 +44 56 06 4.26 B9p:Mn: S:HgMn star.,SB:560.5d, K 2.4k/s, V0 -16.8k/s, asini 16.3. Unresolved by speckle interferometry 1986.45.,VAR:Alpha CV?, 4.23 - 4.27V, amp. 0.015U, 7.832d, symmetric light curve.
HR 6032 BD+10 2971 145589 121414 W 16 11 29.7 +09 42 45 6.53 F0IV 0.0 0.1 D:A5, F1.
HR 6035 BD+17 2982 145647 101994 3279 16 11 28.7 +16 39 56 6.08 A0V
HR 6039 10 BD+23 2909 145713 84240 I LQ Her 16 11 38.0 +23 29 41 5.70 M4.5IIIa VAR:Lb? 5.58 - 5.83V, 7.1 - 7.31p.
HR 6047 9 BD+05 3165 145892 121431 3283 I 16 13 15.4 +05 01 16 5.48 gK5
HR 6050 BD+42 2683 145931 45957 3281 I 9962 16 11 47.6 +42 22 28 5.87 K4II+F6-8V 4.3 23.6 D:Companion, 10.73V, +0.58(B-V), +0.08(U-V), F8IV:, CPM.
HR 6057 BD+06 3184 146084 121443 16 14 13.5 +05 54 07 6.31 K2III
HR 6065 16 BD+19 3075 146388 102040 16 15 28.7 +18 48 30 5.69 K3III
HR 6087 BD+21 2902 147266 84306 16 20 04.3 +21 07 57 6.05 G8IIIb
HR 6090 BD+49 2491 147352 46025 3292 I 16 19 11.2 +49 02 17 5.91 gK6
HR 6091 BD+40 3005 147365 65233 3293 W 16 19 55.1 +39 42 31 5.46 F3IV-V 4.5 2.2 D:CPM.
HR 6092 τ 22 BD+46 2169 147394 46028 608 10010 7641 16 19 44.4 +46 18 48 3.89 B5IV 10.7 6.7 D:ADS 10010AB, 6700y.,VAR:3.85 - 3.90V.
HR 6095 γ 20 BD+19 3086 147547 102107 609 I 10022 7667 16 21 55.2 +19 09 11 3.75 A9III 6.4 41.6 D:ADS 10022B, 9.58v, optical.,G:Hyades group.,SB:11.9d.
HR 6111 21 BD+07 3164 147869 121568 1429 16 24 10.8 +06 56 53 5.85 A2pSr: SB:4.951d, K 16.3k/s, V0 -34.4k/s, asini 0.955.
HR 6117 ω 24 BD+14 3049 148112 102153 613 10054 Ome Her 16 25 25.0 +14 02 00 4.57 B9pCr 8.1 28.4 D:B, 12.0v at 2" CPM; C optical.,G:UMa stream; Sirius group.,N:Kajam; Cujam; Cajam; Caiam.,S:Also classified A2VpCrMnSr.,VAR:Alpha CV, amp. 0.08V, 2.951d, double wave light curve. Also rapid var. 0.15d.
HR 6119 BD+19 3098 148206 102160 I U Her 16 25 47.7 +18 53 33 6.70 M7IIIe S:SiO maser emission. Infrared star showing OH and H2O emission.,VAR:ADS 10449A, M 6.5 - 13.3v, 406.05d.
HR 6121 BD+11 2984 148228 102165 16 26 11.5 +11 24 27 6.11 G8III
HR 6123 25 BD+37 2750 148283 65290 3296 S 16 25 24.2 +37 23 38 5.54 A5V 0.2 S:Shell star.
HR 6146 30 BD+42 2714 148783 46108 3303 I g Her 16 28 38.5 +41 52 54 5.04 M6-III VAR:SRb 4.3 - 6.3v, 5.7 - 7.2p, 89.2d. Also slow var. of about 875d and aperiodic superposed cycles 5 - 15d.
HR 6148 β 27 BD+21 2934 148856 84411 618 I W 7778 16 30 13.2 +21 29 23 2.77 G7IIIa 7.3 256.2 D:Visual companion probably optical.,N:Kornephoros; Korneforos; Rutilicus.,SB:410.575d, K 12.8k/s, V0 -25.5k/s, asini 60.4. Unresolved by speckle interferometry.
HR 6152 BD+20 3283 148897 84416 I 7785 16 30 33.6 +20 28 45 5.25 G8IIICN-2CH-1 G:Wolf 630 group.,S:Also classified G8IIICN-2CH-0.5Ca0.5.
HR 6154 BD+22 2983 149009 84423 I 16 31 13.4 +22 11 43 5.76 gK5
HR 6156 34 BD+49 2514 149081 46128 16 30 06.0 +48 57 39 6.45 A1V
HR 6157 BD+35 2828 149084 65356 3308 I 16 31 02.8 +35 13 30 6.25 K5
HR 6158 28 BD+05 3223 149121 121676 3309 16 32 35.7 +05 31 16 5.63 B9.5III
HR 6159 29 BD+11 3008 149161 102234 3310 I 7812 16 32 36.3 +11 29 17 4.84 K7III VAR:4.82 - 4.85V.
HR 6162 BD+45 2422 149303 46147 10105 16 31 47.3 +45 35 54 5.65 A4Vn 3.3 16.3
HR 6168 σ 35 BD+42 2724 149630 46161 621 S 7837 16 34 06.2 +42 26 13 4.20 B9V 3. 0.1 D:Sep. 0.067". Noted as double by speckle interferometry in 1971-2, unresolved at Mayall 4-meter in 1976. Spectrum,D:double-lined. Resolved by speckle observations 1986.45 (Blazit et al. 1987, A&AS, 71, 57).
HR 6169 BD+17 3053 149632 102259 3313 W 16 35 26.3 +17 03 26 6.41 A2V 1.0 156.6 D:Companion A2V, CPM; vsini 80k/s.,SB:10.56d, K 62.4k/s, V0 -9.9k/s, msin3i 2.20, asini 8.18.
HR 6176 BD+15 3029 149822 102271 V773 Her 16 36 43.0 +15 29 53 6.30 B9pSiCrSr: G:Wolf 630 group.,VAR:Alpha CV, amp. 0.03U, 0.02B, 0.01V, 1.45876d.
HR 6181 BD+13 3177 150012 102278 3316 16 37 48.0 +13 41 13 6.31 F5IV S:Also classified F4V.
HR 6183 BD+46 2194 150030 46184 3314 16 36 11.2 +46 36 48 5.79 G8II
HR 6194 36 BD+04 3234 150379 121774 10149 B 16 40 35.1 +04 12 26 6.93 A3IV 1.2 69.6 D:Binary with HR 6195. Component B is speckle binary, sep. 0.145". Component C, optical. A companion 0.145" from B,D:discovered by speckle interferometry.
HR 6195 37 BD+04 3235 150378 121776 10149 A 16 40 38.7 +04 13 11 5.77 A1V 1.2 69.6 D:Binary with HR 6194, q.v.
HR 6200 42 BD+49 2531 150450 46210 1434 I 10144 7896 16 38 44.9 +48 55 42 4.90 M2.5IIIab 5.4 25.6 D:Optical.
HR 6203 BD+12 3063 150483 102314 16 40 51.4 +12 23 42 6.08 A3Vn
HR 6208 BD+25 3115 150580 84536 3323 I 16 41 00.6 +24 51 31 6.06 K2
HR 6212 ζ 40 BD+31 2884 150680 65485 I 10157 7915 16 41 17.2 +31 36 11 2.81 G0IV 2.6 1.1 D:ADS 10157AB, 2.90 F9IV, 5.53 G7V, 34.49y, a = 1.355". ADS 10157A*, 10.5y, a = 0.08".,DYN:0.096".,G:Zeta Her group.,SB:ADS 10157A, 34.417y D, K 3.8k/s, V0 -69.9k/s, asini 590. Resolved by speckle interferometry.,VAR:ADS 10157A is var. suspect NSV 7915.
HR 6213 39 BD+27 2668 150682 84543 S 16 41 36.7 +26 55 01 5.92 F2III 0.1 SB:2.3076d, K 100.6k/s, V0 -9.0k/s, msin3i 1.14, asini 3.19.
HR 6220 η 44 BD+39 3029 150997 65504 626 I W 7934 16 42 53.8 +38 55 20 3.53 G7.5IIIbFe-1 113.5 D:Companion questioned.
HR 6222 BD+34 2830 151087 65512 3330 16 43 51.7 +34 02 20 5.99 F2-3III-IV
HR 6227 BD+16 3013 151203 102365 I 7950 16 45 22.5 +15 44 43 5.56 M3IIIab
HR 6228 43 BD+08 3271 151217 121843 3332 I W 7952 16 45 49.9 +08 34 57 5.15 K5III 3.9 82.5
HR 6230 BD+43 2642 151388 46262 I 16 45 11.7 +43 13 02 6.05 K4III
HR 6234 45 BD+05 3272 151525 121865 3333 W V776 Her 16 47 46.4 +05 14 48 5.24 B9pCr: 5.2 122.7 G:Possible Pleiades group.,S:Oxygen deficient relative to magnesium.,VAR:Alpha CV, 5.21 - 5.27V, amp. 0.04U, 1.31159d.
HR 6239 BD+13 3225 151627 102393 16 48 08.9 +13 35 26 6.35 G5III
HR 6242 BD+42 2749 151732 46288 3336 I V636 Her 16 47 19.8 +42 14 20 5.87 M4+III-IIIa VAR:Lb 5.83 - 6.03V.
HR 6246 BD+13 3233 151862 102410 10225 16 49 34.6 +13 15 41 5.91 A1V 4.0 5.3
HR 6250 47 BD+07 3256 151956 121895 7990 16 50 19.4 +07 14 52 5.49 A3m G:Possible Eggen group with HR 63, q.v.,VAR:5.5 - 5.54V.
HR 6254 52 BD+46 2220 152107 46305 10227 V637 Her 16 49 14.2 +45 59 00 4.82 A2VpSrCrEu v 4.6 1.8 D:BC 9.0, 9.1, 56.75y, a = 0.267". AxBC physical.,DYN:0.024".,G:Sirius group. UMa stream.,S:Oxygen deficient relative to magnesium. Magnetic star, also classified A3VpSrCrEuMn.,VAR:ADS 10227A, Alpha CV 4.78 - 4.83V, 3.8567d. K line varies, 3.88d.
HR 6256 BD+43 2654 152153 46311 16 49 40.5 +43 25 50 6.13 K0IV
HR 6258 50 BD+30 2884 152173 84641 3339 I 16 50 39.0 +29 48 24 5.72 M1IIIa
HR 6259 BD+32 2795 152224 65595 16 50 43.1 +32 33 13 6.13 K0III
HR 6264 BD+42 2753 152262 46317 16 50 36.1 +41 53 48 6.29 gK3
HR 6268 49 BD+15 3066 152308 102435 629 V823 Her 16 52 04.9 +14 58 27 6.52 B9.5pCr:
HR 6270 51 BD+24 3069 152326 84651 1440 I 16 51 45.3 +24 39 23 5.04 K0.5IIIaCa0.5
HR 6279 53 BD+31 2925 152598 65627 1441 W 16 52 58.1 +31 42 06 5.32 F0-2V 6.7 70.9
HR 6286 BD+47 2400 152812 46349 I S 16 53 17.6 +47 25 01 6.00 K2III 0.3
HR 6287 BD+21 3002 152815 84687 3343 16 54 55.2 +20 57 31 5.41 G8III
HR 6290 BD+13 3258 152830 102474 V644 Her 16 55 16.0 +13 37 11 6.34 F3V s S:Previously classified F5II, unusual luminosity for Delta Sct type var.,SB:11.848d, K 28.5k/s, V0 -3.7k/s, asini 4.41.,VAR:Delta Sct 6.32 - 6.36V, 0.11505449d.
HR 6292 56 BD+25 3156 152863 84692 10259 16 55 02.1 +25 43 50 6.08 G5III 4.6 17.9 D:CPM.,G:Sirius group? UMa stream.
HR 6293 54 BD+18 3266 152879 102476 I 10262 16 55 22.2 +18 26 00 5.35 K4III 4.2 2.5 D:AC, CPM. C, 12.5v at 93".
HR 6301 BD+14 3155 153226 102496 3346 16 57 32.0 +13 53 03 6.37 K0V M:Possible nearby star on basis of spectroscopic parallax.
HR 6305 57 BD+25 3166 153287 84720 16 57 31.0 +25 21 10 6.28 gG5
HR 6306 BD+50 2345 153299 30161 I 16 56 06.4 +50 02 20 6.56 M2IIIab
HR 6307 BD+24 3095 153312 84726 3347 16 57 42.3 +24 22 53 6.32 K0III
HR 6313 BD+42 2774 153472 46401 3349 16 57 50.2 +42 30 45 6.34 K3III
HR 6324 ε 58 BD+31 2947 153808 65716 634 17 00 17.4 +30 55 35 3.92 A0V SB:4.0235d, K 70.7k/s, V0 -24.2k/s, msin3i 1.56, asini 3.91.
HR 6325 BD+22 3045 153834 84758 I 17 00 58.1 +22 37 56 5.65 gK3
HR 6326 BD+15 3095 153882 102536 10310 V451 Her 17 01 33.0 +14 56 58 6.31 B9pCrEu v 4.6 19.0 D:Fixed sep.,VAR:ADS 10310A, Alpha CV 6.26 - 6.34V, 6.00925d. Spectrum, magnetic field, RV, same period. Rotation 6.0087d.
HR 6328 BD+27 2738 153897 84765 17 01 09.6 +27 11 47 6.55 F5V
HR 6332 59 BD+33 2817 154029 65736 1446 17 01 36.4 +33 34 06 5.25 A3IV
HR 6333 BD+25 3183 154084 84776 3356 17 02 18.7 +25 30 20 5.75 gG7
HR 6336 BD+32 2835 154126 65745 17 02 17.2 +31 53 05 6.36 K0
HR 6337 BD+14 3179 154143 102553 I 8142 17 03 07.8 +14 05 31 4.98 M3III G:Gamma Leo group.
HR 6339 BD+14 3180 154160 102554 8143 17 03 10.4 +14 30 40 6.52 G5IV:
HR 6341 BD+13 3292 154228 102564 W 8152 17 03 39.3 +13 36 19 5.93 A1V 0.2 299.2
HR 6342 BD+13 3295 154278 102569 17 03 58.0 +13 34 03 6.08 K1III D:Component B of system with HR 6341.,G:Gamma Leo group.
HR 6343 BD+19 3218 154301 102571 I 10323 8158 17 03 52.7 +19 41 26 6.35 K4III 4.3 108.1 D:B, 11.0v at 1.5" CPM.,VAR:ADS 10323B, 10 - 11.3v?
HR 6346 61 BD+35 2911 154356 65761 I 8159 17 03 30.2 +35 24 51 6.69 R M4IIIab
HR 6351 BD+34 2890 154431 65766 17 03 53.5 +34 47 25 6.04 R A5V
HR 6352 BD+19 3220 154441 102579 10326 17 04 41.3 +19 35 57 6.17 R B9.5V 3.0 1.9
HR 6355 60 BD+12 3142 154494 102584 635 10334 17 05 22.7 +12 44 27 4.91 A4IV 6.1 56.0 D:Optical.,G:Possible Eggen group with HR 63, q.v.
HR 6362 BD+44 2652 154713 46478 1448 17 05 05.0 +43 48 44 6.43 A3IV
HR 6363 BD+49 2583 154732 46476 3359 8185 17 04 49.8 +48 48 15 6.09 K1III G:Gamma Leo group.,SB:786d, K 10.0k/s, V0 +12.8k/s, asini 103.,VAR:6.7 - 6.9p.
HR 6364 BD+22 3073 154733 84835 3360 I 10343 17 06 18.1 +22 05 03 5.56 K3III 7.9 30.3 D:Optical.
HR 6376 BD+40 3103 155102 46502 636 17 07 46.7 +40 30 58 6.34 A2IV
HR 6377 BD+36 2827 155103 65812 10360 17 08 02.0 +35 56 07 5.39 A5-F1III/IVm s 0.1 0.1 D:AB 6.2 A9III-IV, 6.2 A9III-IV, 8.159y, a = 0.116". Mean mass 2.7 solar. Alternate orbit, 16.08y, a = 0.167". Combined,D:colors. Speckle interferometry indicates companion 1 mag. fainter than primary at 0.079". However, speckle,D:observations 1986.46 (at 7000 Ang.) give sep. 0.15".,DYN:0.017".,S:K/H/met give A5/F0V/F2.
HR 6388 BD+40 3109 155410 46524 3365 I S 17 09 33.3 +40 46 38 5.08 K3III SB:876.25d, K 4.79k/s, V0 -57.58k/s, asini 45.8. Unresolved at 10 epochs between 1977.69 and 1981.47 with sep. 0.039",SB:on 1980.48 (McAlister and Hartkopf).
HR 6391 63 BD+24 3140 155514 84896 V620 Her 17 11 03.2 +24 14 16 6.19 A8V VAR:Delta Sct 6.19 - 6.23V. Period analyses of new and existing data by Reed and Welch (1988, AJ, 95, 1510) favor,VAR:fundamental period of 0.088d with overtones of 0.052, 0.130d, with the fundamental and second values as radial,VAR:pulsations and the third as nonradial.
HR 6399 BD+49 2604 155860 46561 10397 8327 17 11 40.2 +49 44 48 6.04 R A5III 3.4 5.2 D:AB, CPM.
HR 6406 α1 64 BD+14 3207 156014 102680 I 10418 A Alp Her 17 14 38.9 +14 23 25 3.48 H M5Ib-II e 2.2 4.9 D:AB, 3600y, a = 4.68". Component B is HR 6407. Combined colors. Combined mag. 3.08V. Mass A, 14 solar. Other components,D:faint, optical. Circumstellar lines around both A, B.,DYN:0.008".,N:RASALGETHI; Ras Algethi; Rasalegti.,R:Diam. = 0.020 - 0.030".,S:Ultraviolet FeII emission. 5-micrometer observations indicate carbon monoxide.,VAR:ADS 10418A. Discovered by W. Herschel in 1795. SRc 3.0 - 4.0v. 6-yr. period superimposed by variations 50 - 155d.,VAR:Surrounded by envelope of 2x10E+05 solar radii, expanding 10k/s, mass loss 3x10E-08 solar masses/y.
HR 6407 α2 64 BD+14 3207 156015 102681 10418 B 17 14 39.2 +14 23 24 5.39 H G5III+F2V 2.2 4.9 C:IR source.,D:See HR 6406.,DYN:0.008".,SB:51.578d, K 36.1k/s, V0 -38.4k/s, asini 25.6. Sp. of fainter comp. of the SB, A3V, may be a collapsed star. Masses,SB:4.1, 2.5 Suns.
HR 6410 δ 65 BD+25 3221 156164 84951 641 I 10424 8419 17 15 01.9 +24 50 21 3.14 A3IV 5.6 8.5 D:ADS 10424B, dG4, optical.,N:Sarin.
HR 6418 π 67 BD+36 2844 156283 65890 643 I 8431 17 15 02.8 +36 48 33 3.16 K3IIab e G:Red star Pleiades group.,S:Ultraviolet FeII emission.
HR 6419 BD+23 3070 156284 84955 I 17 15 41.6 +23 44 34 5.96 K2III
HR 6430 BD+23 3074 156593 84982 I 17 17 35.9 +23 05 27 6.45 R K2
HR 6431 68 BD+33 2864 156633 65913 10449 u Her 17 17 19.5 +33 06 00 4.82 B1.5Vp+B5III 5.1 4.4 D:Binary.,DYN:0.010".,SB:ADS 10449A, B2.5V, B5V, 2.0510d, K 95.6k/s, V0 -30.0k/s, msin3i 7.16, asini 2.69. Semi-detached system. vsini of,SB:secondary 88k/s.,VAR:ADS 10449A, EA 4.69 - 5.37V, 2.0510270d. i 75.9d. Semi-detached system. Polarization measures indicate light from,VAR:primary reflected on photosphere of secondary.
HR 6432 BD+17 3216 156653 102724 17 18 05.0 +17 19 05 6.00 A1V
HR 6436 69 BD+37 2864 156729 65921 8489 17 17 40.3 +37 17 30 4.65 A2V
HR 6437 BD+49 2614 156753 46605 17 16 48.6 +49 41 28 7.48 R K2
HR 6443 BD+28 2719 156874 85001 3375 17 18 48.5 +28 49 23 5.65 K0III
HR 6444 BD+38 2910 156891 65930 3373 17 18 23.3 +38 48 41 5.94 gG7
HR 6452 BD+18 3351 157049 102757 1454 I V656 Her 17 20 18.9 +18 03 26 5.00 M2IIIab VAR:Lb? 4.9 - 5.1v, amp. 0.16p.
HR 6455 BD+25 3246 157087 85016 17 20 09.8 +25 32 15 5.38 A3III
HR 6457 70 BD+24 3167 157198 85021 W 17 20 54.2 +24 29 58 5.12 A2V 3.5 222.9
HR 6458 72 BD+32 2896 157214 65963 1456 10488 8553 17 20 39.6 +32 28 04 5.39 G0V 5.1 230.0 D:B not CPM; optical.,VAR:Amp. 0.4V.
HR 6463 BD+16 3163 157257 102770 I 17 21 33.4 +16 43 51 6.35 M2.5IIIab
HR 6464 74 BD+46 2293 157325 46645 3377 I 8556 17 20 21.1 +46 14 27 5.59 M0III G:61 Cyg group.
HR 6466 BD+28 2728 157358 85028 W 17 21 31.2 +28 45 29 6.35 G0III 2.2 0.6
HR 6467 BD+48 2506 157373 46651 17 20 33.6 +48 11 18 6.43 F4V
HR 6469 BD+40 3136 157482 46664 S V819 Her 17 21 43.6 +39 58 28 5.51 F9Vn: e 0.0 D:Recognized as triple system by speckle interferometry: single star G5IV and close pair of which the brighter component,D:is F7V eclipsing, sep. 0.045".,S:Also classified F7V?+G5IV. Weak H alpha emission.,SB:5.53y.,VAR:E, amp. 0.085V, 2.2299d. Also long period var. outside eclipse, amp. 0.04V, 83.2d; probably the rotation period of,VAR:the G5IV component.
HR 6480 73 BD+23 3100 157728 85062 3383 8606 17 24 06.6 +22 57 37 5.74 F0IV VAR:Delta Sct?
HR 6481 BD+16 3174 157740 102805 17 24 31.5 +16 18 04 5.71 A3V G:Sirius group?
HR 6482 BD+15 3179 157741 102806 10528 17 24 33.8 +15 36 22 6.35 B9V 4.3 3.9 D:Fixed sep. Companion A6V, optical.
HR 6484 ρ 75 BD+37 2878 157778 66000 10526 B 17 23 40.7 +37 08 48 5.47 H A0Vn 1.0 4.2 D:Binary with HR 6485, q.v. Another companion with sep. 0.29" seen on 1981.47 (McAlister and Hartkopf). Unresolved on,D:1985.25 (Bonneau et al.).,DYN:0.010".
HR 6485 ρ 75 BD+37 2878 157779 66001 10526 A 8605 17 23 41.0 +37 08 45 4.52 H B9.5III 1.0 4.2 D:Binary with HR 6484. Combined colors. Combined mag. 4.17V.,DYN:0.010".,S:Silicon star.,VAR:ADS 10526A, E?
HR 6488 BD+38 2928 157853 66006 10531 17 24 02.2 +38 34 58 6.49 F8IV 0.1 0.1 D:dF7, CPM, sep. 0.100". Measured sep. 0.069" on 1985.5 by speckle interferometry.
HR 6491 BD+37 2882 157910 66014 10535 17 24 27.1 +36 57 07 6.28 G5III+F0V 3.6 33.2 D:F0V, CPM.
HR 6495 BD+17 3241 157967 102819 I W V640 Her 17 25 54.4 +16 55 03 5.98 M4IIIab 7.5 23.1 VAR:Lb 5.98 - 6.21V.
HR 6499 BD+27 2809 158067 85080 3387 W 17 26 00.9 +26 52 44 6.41 A5IV 5.0 49.4
HR 6502 BD+20 3481 158148 85095 3388 17 26 49.1 +20 04 51 5.54 B5V
HR 6506 BD+34 2971 158261 66054 3389 17 26 46.2 +34 41 45 5.94 A0V SB:5.9182d, K 25.1k/s, V0 -22.7k/s, asini 2.04.
HR 6509 77 BD+48 2517 158414 46723 650 17 26 44.2 +48 15 36 5.85 A4V
HR 6526 λ 76 BD+26 3034 158899 85163 1460 I 9070 17 30 44.3 +26 06 38 4.41 K3.5III N:Maasym; Masym; Misam, a name also applied to h and Chi Per.
HR 6528 BD+31 3047 158974 66103 17 30 55.4 +31 09 30 5.61 G8III
HR 6531 BD+39 3147 159026 66102 17 30 40.3 +38 52 56 6.43 F6III
HR 6533 78 BD+28 2767 159139 85182 17 31 49.6 +28 24 27 5.62 R A1V
HR 6538 BD+34 2989 159222 66118 17 32 01.1 +34 16 15 6.56 G5V G:Theta Cen group.
HR 6541 BD+19 3354 159332 102912 3393 17 33 22.8 +19 15 24 5.64 F6V
HR 6542 BD+16 3218 159353 102917 3394 17 33 39.4 +16 19 03 5.69 gK0
HR 6543 BD+14 3279 159354 102918 I V642 Her 17 33 42.8 +14 50 30 6.48 M4IIIa VAR:SRb 6.41 - 6.56V, about 12d.
HR 6550 BD+41 2850 159501 46792 1462 17 33 07.3 +41 14 37 5.74 gK1
HR 6551 BD+16 3220 159503 102928 17 34 27.2 +16 30 14 6.40 R A8Vn
HR 6559 BD+21 3157 159834 85232 10655 17 35 59.6 +20 59 46 6.10 A7IV 3.5 10.4 D:Companion, 9.53V, +0.36(B-V), -0.02(U-B), F6IV-V, CPM.
HR 6563 BD+37 2908 159925 66165 3395 17 35 42.4 +37 18 06 6.10 G9III
HR 6564 BD+28 2787 159926 85236 17 36 07.9 +28 11 05 6.38 R K5
HR 6570 BD+30 3033 160054 66175 3397 17 36 36.7 +30 47 07 6.02 A5V
HR 6571 79 BD+24 3218 160181 85264 3400 S 17 37 31.1 +24 18 36 5.77 A2Vn 0.1
HR 6574 82 BD+48 2542 160290 46838 I 17 36 37.6 +48 35 08 5.37 gK1
HR 6579 BD+32 2964 160507 66214 17 38 49.7 +32 44 22 6.37 R gG5
HR 6584 BD+31 3075 160677 66231 I 17 39 57.5 +31 12 09 6.03 M2IIIab
HR 6588 ι 85 BD+46 2349 160762 46872 663 W Iot Her 17 39 27.9 +46 00 23 3.80 B3IV 8.3 116.0 C:Color excess E(B-V) = -0.02.,SB:113.804d, K 5.4 k/s, V0 -20.0 k/s, asini 7.629. RV also var. 0.1434d.,VAR:Beta C?, amp. 0.01V.
HR 6589 BD+15 3246 160765 103020 17 41 11.0 +15 10 41 6.34 A1V
HR 6591 BD+31 3076 160822 66243 W 17 40 41.2 +31 17 15 6.28 K0III 2.1 115.0
HR 6592 BD+24 3225 160835 85310 10715 17 41 05.5 +24 30 48 6.36 K1III+F4V 3.0 16.3 D:Component B, F4V CPM.
HR 6594 BD+16 3256 160910 103033 10723 17 41 58.7 +15 57 07 5.52 F4V w 2.8 0.6 D:AB 5.58 F4V, 11.1, 122.68y, a = 1.004". Component C, 12.8v at 155" CPM.,DYN:0.030".
HR 6599 BD+43 2781 160950 46883 17 40 37.6 +43 28 15 6.59 R K2
HR 6602 83 BD+24 3231 161074 85344 I W 17 42 28.4 +24 33 51 5.52 K4III 3.6 159.6
HR 6604 BD+14 3321 161149 103052 3407 17 43 22.0 +14 17 42 6.24 F5II G:Hyades group.,S:Also classified F4IV, Sr enhanced; F2III and F4V.,VAR:Delta Sct?
HR 6608 84 BD+24 3237 161239 85360 17 43 21.6 +24 19 40 5.71 G2IIIb
HR 6611 BD+14 3329 161321 103069 10749 V624 Her 17 44 17.3 +14 24 37 6.19 A3m 5.7 39.7 D:Visual companion ADS 10749B, optical.,S:Also classified A3pSiSr and A2.5/A7/F0.,SB:ADS 10749A, 3.894977d, K 96.6k/s, V0 -32.4k/s, msin3i 1.83, asini 5.17. Both components Am. vsini 35 and 30k/s.,VAR:EA 6.18 - 6.36V, 3.894977d.
HR 6612 BD+44 2757 161369 46906 3408 I 17 43 05.6 +44 05 04 6.34 K4III
HR 6619 BD+31 3090 161695 66311 3410 17 45 40.3 +31 30 17 6.23 A0Ib
HR 6623 μ 86 BD+27 2888 161797 85397 667 I 10786 17 46 27.5 +27 43 14 3.42 G5IV 6.4 33.8 D:BC 10.3 dM4, 10.8, 43.20y, a = 1.360". This close pair forms a wider physical binary with component A.,DYN:0.132".,G:Wolf 630 group.
HR 6625 BD+38 2997 161815 66315 3411 17 45 53.7 +38 52 53 6.52 K0
HR 6626 BD+39 3219 161832 66317 10782 V826 Her 17 45 58.5 +39 19 21 6.68 K3III+F7V 3.1 7.9 D:Component B, 9.70V, +0.75(B-V), +0.19(U-B), F5V, binary. Component C mag. diff 5.36v at 70" from A.,SB:ADS 10782A, 99.557d, K 16.45k/s, V0 -26.72k/s, asini 22.52.
HR 6627 BD+17 3334 161833 103106 10795 17 47 08.0 +17 41 50 5.72 R A1V 1.3 0.6 D:Binary.
HR 6638 BD+20 3570 162076 85429 1465 17 48 24.8 +20 33 56 5.69 G5IV
HR 6641 BD+47 2537 162132 46954 S 17 47 08.1 +47 36 44 6.43 A2V s 0.1 SB:2.8242d, K 60.2k/s, V0 -27.1k/s, asini 2.34.
HR 6642 BD+19 3435 162161 103131 17 48 47.9 +19 15 19 6.12 A1V
HR 6644 87 BD+25 3353 162211 85437 3415 I 17 48 49.2 +25 37 22 5.12 K2III
HR 6654 BD+29 3126 162555 85464 17 50 22.9 +29 19 20 5.50 K1III
HR 6655 BD+22 3227 162570 85468 17 50 48.4 +22 18 59 5.98 R A9V
HR 6664 88 BD+48 2581 162732 46997 3417 V744 Her 17 50 03.3 +48 23 39 6.68 BepShell v S:H alpha emission.,SB:86.59d, K 9.7k/s, V0 -11.6k/s, asini 11.4. Companion 1 solar mass at about 150 solar radii.,VAR:Gamma Cas 6.65 - 6.94V, 86.7207d, similar to Pleione (HR 1180). Spectrum var. with possible periods 2.5552 and,VAR:0.78906d, correlated with RV.
HR 6665 BD+15 3292 162734 103161 10850 17 51 58.5 +15 19 33 6.46 R K0III 0.2 0.8 D:AB binary. C, 13v at 28" and D, 10v at 95" both optical.,G:Probable Hyades group.
HR 6669 BD+40 3225 162826 47009 17 51 14.0 +40 04 21 6.46 R G0V
HR 6673 BD+40 3228 162989 66402 3419 I 17 52 04.7 +39 58 56 6.04 gK4
HR 6674 BD+46 2379 163075 47023 17 52 01.0 +46 38 36 6.38 K0III
HR 6677 90 BD+40 3233 163217 47037 I 10875 9834 17 53 18.1 +40 00 29 5.16 K1IIIbCN-1 3.3 1.6 DYN:0.003".,G:Hyades group.,S:If the secondary is a main sequence star, the inferred spectral type is A5V.,VAR:ADS 10875. Not certain which component is the var. suspect. Rapid change in difference between components.
HR 6685 89 BD+26 3120 163506 85545 1468 I V441 Her 17 55 25.2 +26 03 00 5.46 F2Ib e C:IR excess.,RV:About 70d. Mass loss 10E-08 solar masses/y.,S:2- and 10-micrometer spectra show silicate emission indicating circumstellar shell. Infrared emission at wavelengths,S:longer than 2 micrometers probably originates in circumstellar shell of solid particles.,VAR:SRd 5.34 - 5.54V, 68:d.
HR 6687 BD+22 3237 163547 85552 3427 I 17 55 50.8 +22 27 51 5.58 gK3
HR 6695 θ 91 BD+37 2982 163770 66485 672 I 9890 17 56 15.2 +37 15 02 3.86 K1IIaCN+2 e VAR:Possibly 5 yr. period in He 10830 emission.
HR 6697 BD+24 3283 163840 85575 S 17 57 14.3 +23 59 45 6.30 G2V 1.5 0.1 D:Sep. 0.107". Closed from 0.114" to 0.065" between 1981.5 and 1984.3 (McAlister and Hartkopf). However, speckle,D:observations 1986.44 (Blazit et al. 1987, A&AS, 71, 57) yield 0.085".,M:Possible nearby star on basis of spectroscopic parallax.
HR 6702 BD+45 2627 163990 47080 I OP Her 17 56 48.4 +45 21 03 6.02 M5IIbS S:Technetium star.,VAR:SRb 5.85 - 6.73V, 7.7 - 8.3p, 120.5d.
HR 6703 ξ 92 BD+29 3156 163993 85590 674 I 9927 17 57 45.9 +29 14 52 3.70 G8+III
HR 6707 ν 94 BD+30 3093 164136 66524 Nu Her 17 58 30.2 +30 11 22 4.41 F2II S:Manganese star. IUE observations suggest B9.5V companion.,VAR:SRd? 4.38 - 4.48V, 29:d. However, more recent photoelectric observations cast doubt on variability.
HR 6711 BD+36 2986 164280 66531 17 58 42.3 +36 17 16 6.00 gG5
HR 6713 93 BD+16 3335 164349 103285 1469 I 18 00 03.4 +16 45 03 4.67 K0.5IIb G:Red star Pleiades group.,S:Barium star.
HR 6718 BD+45 2635 164429 47106 V771 Her 17 58 52.3 +45 28 34 6.48 B9pSiSr VAR:Alpha CV 6.44 - 6.52V, amp. 0.04U, 0.517468d.
HR 6720 BD+19 3494 164447 103291 Var? 18 00 27.7 +19 30 21 6.50 B8Vne S:Shell star.
HR 6722 BD+15 3327 164507 103299 18 00 57.2 +15 05 36 6.26 G5IV
HR 6726 BD+33 3006 164614 66551 I 18 00 36.4 +33 12 50 5.99 gK6
HR 6728 BD+45 2638 164646 47121 3433 I 9980 17 59 56.2 +45 30 05 5.67 M0IIIab
HR 6729 95 BD+21 3280 164668 85647 I 10993 B 10014 18 01 29.9 +21 35 43 5.18 G8III 0.1 6.3 D:Binary with 6730.,DYN:0.007".
HR 6730 95 BD+21 3280 164669 85648 10993 A 10014 18 01 30.4 +21 35 44 4.96 A5IIIn 0.1 6.3 D:Binary with 6729.,DYN:0.007".
HR 6737 BD+33 3009 164824 66562 3434 I 10998 18 01 35.9 +33 18 41 6.15 K5III 6.0 14.2 D:AB CPM. C, 13v at 55" optical.
HR 6738 96 BD+20 3649 164852 85672 V820 Her 18 02 23.1 +20 50 01 5.28 B3IV RV:12.7d.,SB:12.4573d, K1 57.6k/s, K2 57.5k/s, V0 -15.5k/s, m1sin3i 0.591, m1sin3i 0.592,,SB:a1sin3i 12.0, a2sin3i 12.0.,VAR:5.17 - 5.19B. Observations satisfy the SB period.
HR 6741 97 BD+22 3260 164900 85676 18 02 30.1 +22 55 23 6.21 B3Vn
HR 6744 BD+19 3508 165029 103334 18 03 14.7 +19 36 47 6.50 R A0V
HR 6753 BD+48 2627 165358 47173 11028 18 03 09.0 +48 27 52 6.21 A2V 2.7 26.8 D:Both companions optical.
HR 6754 BD+23 3254 165373 85706 18 04 40.2 +23 56 33 6.34 F0IV-V
HR 6763 BD+21 3300 165524 85718 18 05 30.2 +21 38 49 6.15 gK3
HR 6764 BD+40 3276 165567 47193 18 04 43.2 +40 05 03 6.52 F7V
HR 6765 98 BD+22 3273 165625 85725 I 10208 18 06 01.9 +22 13 08 5.06 M3-IIIZrO 0+
HR 6767 BD+41 2968 165645 47195 11054 18 05 00.8 +41 56 48 6.34 F0V 3.6 23.4
HR 6768 BD+32 3047 165683 66626 18 05 49.6 +32 13 50 5.71 K0III
HR 6775 99 BD+30 3128 165908 66648 11077 18 07 01.5 +30 33 43 5.04 F7V 3.4 1.7 D:AB 5.10 F7V, 8.50 K4V, 55.8y, a = 1.00".,DYN:0.060".,S:Metal deficient, calcium rich.,SB:Astrometric binary unresolved by speckle interferometry.
HR 6779 ο 103 BD+28 2925 166014 85750 681 S Omi Her 18 07 32.6 +28 45 45 3.83 B9.5V e S:H alpha emission.,VAR:Gamma Cas 3.81 - 3.9B, 4.1 - 4.2p.
HR 6781 100 BD+26 3178 166045 85753 11089 A 10253 18 07 49.5 +26 06 05 5.86 A3V 0.0 14.3 D:Binary with HR 6782. Primary is speckle binary, sep. 0.106". Component C, 11v at 76". A companion to A at 0.106",D:discovered by speckle interferometry.,VAR:Combined light of 6781-2 varies; uncertain which component the variable.
HR 6782 100 BD+26 3178 166046 85752 11089 B 10253 18 07 49.5 +26 05 51 5.90 A3V 0.0 14.3 D:Binary with HR 6781.
HR 6787 102 BD+20 3674 166182 85769 3443 11102 18 08 45.5 +20 48 52 4.36 B2IV 7.9 23.4 D:Companion A6V, optical.
HR 6791 BD+43 2892 166208 47237 I 18 07 28.8 +43 27 42 5.00 G8IIICN-1CH-3
HR 6792 BD+49 2732 166228 47233 11090 18 07 06.3 +49 42 38 6.32 R A2V 4.1 2.4
HR 6793 BD+36 3027 166229 66666 I 18 08 02.2 +36 24 05 5.48 K2.5III
HR 6794 101 BD+20 3675 166230 85770 18 08 52.9 +20 02 43 5.10 A8III
HR 6799 BD+30 3138 166411 66682 18 09 10.2 +30 28 10 6.38 gK1
HR 6803 BD+16 3390 166479 103443 11123 10311 18 10 08.7 +16 28 36 6.09 R B9V+F7III 0.8 1.2 D:6.5 A, 7.2 F2, 3040y, a = 1.500".,S:Also classified G2III + A0V:.
HR 6806 BD+38 3095 166620 66700 10316 18 09 37.5 +38 27 27 6.40 K2V G:Wolf 630 group.
HR 6807 BD+36 3039 166640 66703 18 09 59.0 +36 27 59 5.58 G8III
HR 6814 BD+33 3044 166988 66733 11149 10363 18 11 45.1 +33 26 49 5.88 R A3V 0.3 0.1 D:AB measured sep. 0.102" on 1985.5 by speckle interferometry.,SB:ADS 11149A.,VAR:ADS 11149B, 8.5 - >11?v.
HR 6815 104 BD+31 3199 167006 66737 3448 I V669 Her 18 11 54.2 +31 24 19 4.97 M3III VAR:Amp. 0.14B.
HR 6820 BD+21 3347 167193 85836 I 18 13 16.5 +21 52 49 6.12 K4III
HR 6824 BD+41 3011 167304 47305 18 12 42.6 +41 08 49 6.36 K0III
HR 6826 BD+38 3113 167370 66765 3451 18 13 04.8 +38 46 25 6.04 B9IIIn
HR 6831 BD+29 3213 167588 85856 18 14 44.0 +29 12 26 6.56 F8V
HR 6852 BD+18 3623 168270 103581 18 18 07.7 +18 07 53 5.99 R B9V
HR 6854 BD+23 3299 168323 85906 I W 18 18 07.7 +23 17 48 6.63 R K5 2.3 155.4
HR 6860 105 BD+24 3381 168532 85921 3457 I 18 19 10.7 +24 26 46 5.27 K3III:Ba0.4 SB:478d, K 16.1k/s, V0 -14.4k/s, asini 97.0.
HR 6867 BD+29 3236 168694 85933 I 18 19 52.1 +29 39 58 5.99 gK4
HR 6868 106 BD+21 3390 168720 85941 I 18 20 17.9 +21 57 41 4.95 M1III
HR 6876 108 BD+29 3241 168913 85956 18 20 57.1 +29 51 32 5.63 A5m SB:5.5146d, K 70.1k/s, V0 -20.2k/s, msin3i 1.72, asini 5.32. vsini both components 20k/s.
HR 6877 107 BD+28 2981 168914 85957 10690 18 21 01.0 +28 52 12 5.12 A7V
HR 6882 BD+23 3316 169110 85975 I 18 22 08.7 +23 17 07 5.41 M0IIIab
HR 6885 BD+17 3555 169191 103655 3460 I 18 22 49.0 +17 49 36 5.25 K3III
HR 6887 BD+16 3478 169223 103660 18 23 02.9 +16 41 17 6.22 K0
HR 6895 109 BD+21 3411 169414 86003 690 I W 10742 18 23 41.9 +21 46 11 3.84 K2.5IIIab 6.5 221.8
HR 6904 BD+27 3016 169718 86019 11334 18 24 58.5 +27 23 43 6.27 A0V+A4V 0.9 0.6 D:AB 6.5 A2V, 7.5 A4V, 775y, a = .90".,SB:ADS 11334A.
HR 6906 BD+14 3533 169820 103709 S 18 25 55.4 +14 58 00 6.37 B9V 0.1
HR 6917 BD+29 3259 169981 86043 1479 18 25 58.8 +29 49 44 5.83 A2IV G:Sirius group; UMa stream.,SB:9.6120d, K 28.5k/s, V0 +7.5k/s, asini 3.32.
HR 6924 BD+26 3259 170111 86060 11356 18 26 40.9 +26 26 58 6.53 B3V 2.7 62.3 D:B, 12.6v at 6". Possibly CPM and common RV with HD 170051, 6.9v B5 at 185".,SB:ADS 11356A.
HR 6943 BD+23 3347 170650 86115 18 29 35.7 +23 51 58 5.90 B6IV
HR 6950 BD+20 3821 170829 86142 Var? 18 30 41.6 +20 48 55 6.50 G8IV SB:26.390d, K 12.4k/s, V0 -59.0k/s, asini 4.43.
HR 6955 BD+16 3529 170878 103800 1481 18 31 04.4 +16 55 43 5.77 A2V
HR 6966 BD+23 3363 171245 86175 3472 I W 18 32 46.2 +23 37 01 5.84 gK5 D:Suspected binary probably single star.
HR 6975 BD+20 3847 171487 86203 3476 18 34 19.6 +20 27 59 6.57 A3V
HR 6977 BD+18 3740 171623 103879 S 18 35 12.6 +18 12 12 5.78 R A0Vn 0.2
HR 6980 BD+23 3385 171745 86224 11479 18 35 30.4 +23 36 20 5.61 G9III+G7III 0.2 0.6 D:6.3 G9III, 6.5 G7III, 210.9y, a = 0.416" or 190.8y, a = 0.418". Combined mag., colors.
HR 6981 BD+16 3560 171746 103886 11483 11085 18 35 53.2 +16 58 32 6.21 G2V+G2V 0.2 1.8 D:AB 6.8 G2V, 7.0 G2V, 292y, a = 1.358", or 3083y, a = 6.7811".,DYN:0.024".,S:AB also classified F8V.
HR 6995 BD+16 3563 171994 103913 18 37 09.0 +16 11 54 6.29 G8IV
HR 7047 BD+23 3439 173494 86393 18 44 40.2 +23 35 23 6.31 F6V
HR 7058 BD+21 3550 173650 86405 V535 Her 18 45 35.7 +21 59 06 6.51 B9pSiCr: v S:Si star. Enhanced chromium, iron, titanium, strontium.,VAR:Alpha CV 6.41 - 6.58V, 10.1353d or 9.975d; also spectrum, magnetic field, RV.
HR 7061 110 BD+20 3926 173667 86406 703 I 11658 11323 18 45 39.7 +20 32 47 4.19 F6V 9.2 63.8 D:All companions probably optical.
HR 7067 BD+18 3817 173833 104087 I 18 46 41.4 +18 42 21 6.17 K5
HR 7069 111 BD+18 3823 173880 104093 1491 W 18 47 01.3 +18 10 53 4.36 A5III 5.5 121.3 G:Hyades group.
HR 7079 BD+23 3461 174160 86451 18 48 16.4 +23 30 51 6.15 F8V M:Possible nearby star on basis of spectroscopic parallax.
HR 7086 BD+19 3798 174262 104129 18 48 53.4 +19 19 43 5.88 A1V
HR 7091 BD+24 3545 174369 86462 S 18 49 14.4 +25 02 47 6.59 R A1V 0.2 SB:13.081d, K 28.9k/s, V0 -25.9k/s, asini 4.79.
HR 7109 BD+13 3787 174853 104196 3503 S V822 Her 18 52 01.9 +13 57 56 6.14 B8Vnn 0.1 S:nn spectral type probably due to unresolved double lines on classification plates (Hube et al. 1988, AJ, 95, 199).,S:Spectral type of secondary similar to that of primary (late B). vsini of primary and secondary 96 and 91k/s,,S:respectively.,SB:1.391113d, K 165.8k/s, V0 -24.1k/s, msin3i 2.63, asini 3.17.,VAR:EB 6.12 - 6.30V.
HR 7113 112 BD+21 3582 174933 86521 18 52 16.4 +21 25 31 5.48 B9II-IIIpHg G:Possible Pleiades group.,S:HgMn star. Spectrum shows phosphorus. Gallium II lines strong.,SB:6.3624d, K 17.7k/s, V0 -19.6k/s, asini 1.54.
HR 7133 113 BD+22 3524 175492 86567 3508 I 11820 18 54 44.9 +22 38 42 4.59 G4III+A6V 7.9 35.7 D:C, 11v at 38" optical.,S:Also classified G5III + A2V.,SB:ADS 11820A, 245.3d, K 16.0k/s, V0 -23.3k/s, asini 53.6. Binary motion corresponds to the G-type spectrum; the A,SB:type arises from an unresolved companion, vsini 60k/s.
HR 7147 BD+17 3778 175744 104271 V828 Her 18 56 03.9 +17 59 42 6.63 B9pSi G:Member of Pleiades group.
HR 7148 BD+17 3779 175743 104272 18 56 06.2 +18 06 19 5.69 K1III G:Gamma Leo group.

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