Catalogues

Camelopardalis / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HRBFDMHDSAOFK5IRM*ADSVarIDRADecvMagspTypedMagSepRemarks
HR 967BD+65 33820104126862436 03 17 31.6+65 39 316.36 A3V 0.40.5D:AB 6.8 A2V, 7.3 A4V, 330y, a = 0.386". Combined mag., colors.,RV:Discordant sign from only two available sources, -7.5, +6.4.
HR 985BD+65 3402033612704W BK Cam03 19 59.4+65 39 084.84 B2.5Ven v7.7120.9D:Probably optical.,G:Cas-Tau OB1.,S:Shell star.,SB:4.5y.,VAR:Gamma Cas, 4.78 - 4.89V. Spectrum var. 4.5y from 1916 to 1931, previously longer cycles, but no changes noted after,VAR:1937. R-I also found at -0.03 and -0.05.
HR 1009BD+64 39120797127431096I 1121 03 24 40.5+64 35 105.23 M0II
HR 1033BD+59 65721203127702538 03 28 23.6+60 15 206.49 B9V+A1 1.00.2D:AB 6.8 B9V, 7.8 A1V, 259.90y, a = 0.370". Combined mag., colors.
HR 1035BD+59 66021291240541222544 1152 03 29 04.1+59 56 254.21 B9Ia 4.32.4G:Cam OB1; in reflection nebula; member assoc. Cam R1 at 870 pc.,VAR:H alpha profile var.
HR 1040BD+58 6072138924061I 03 29 54.9+58 52 434.54 A0Ia eG:Cam OB1; in reflection nebula; member assoc. Cam R1 at 870 pc.,VAR:H alpha profile variable.
HR 1043BD+58 60821427240622563 1158 03 30 11.3+59 21 586.13 A2V 1.42.5
HR 1046BD+54 68421447240642565 1159 03 30 00.2+55 27 075.09 A1V 4.814.8D:AB CPM.,G:UMa stream. Possible Eggen group with HR 63, q.v.,VAR:Delta Sct.
HR 1068BD+58 61921769240932592 A03 33 32.1+58 45 546.40 A4III 1.720.4D:AB CPM. B, spectral class F2V. Component C, 10.5v at 164".,S:Also classified Am(A3/A7/F0).
HR 1071BD+57 73021794240982252 03 33 41.2+57 52 086.37 F7V
HR 1073BD+54 6932181924099 03 33 39.0+54 58 295.98 A3V
HR 1077BD+59 67521903241112612 03 35 00.8+60 02 286.46 F3V 0.91.1D:AB 6.8 F3V, 7.6 F9V, 287.7y, a = 1.245". Combined mag., colors. Mass AB, 2.2 solar. C, 10.3v at 92" optical.
HR 1094BD+56 8262231624133 03 38 19.7+56 55 586.30 B9p vVAR:Spectrum variable.
HR 1105BD+62 5972264912874129I BD Cam03 42 09.3+63 13 005.10 S3.5/2 S:Technetium not abundant, as previously reported.,VAR:Lb 5.04 - 5.17V, 6.7 - 6.85p.
HR 1112BD+59 6992276424169I2691 03 42 42.7+59 58 105.76 K3IIb 2.454.7D:Component D, 8.73V, +0.10(B-V), -0.22(U-B), B8III.,S:Spectrum formerly classified as K4Ib. According to P. C. Keenan (October 1986), recent spectrograms, although not of,S:extremely high quality, show that star is not as luminous as Ib, with best spectral type of S. Yorka and P. C.,S:Keenan reported as K3IIb, although it may be slightly later.
HR 1124BD+66 28423005128902267 03 46 00.9+67 12 065.80 F0IV
HR 1129BD+62 6042308912891IS 03 46 02.3+63 20 424.80 G0III+A3V 1.00.1D:5y? Sep. 0.052". vsini of secondary =<50k/s.,S:Also classified G2II-III + B9V.,SB:219.971d, K 39.15k/s, V0 -18.38k/s, asini 118.
HR 1138BD+70 257232775000 03 49 13.8+70 52 165.44 A2m SB:15.5132d, K 22.2k/s, V0 +16.0k/s, msin3i 0.0813, asini 4.62. vsini both components 25k/s.
HR 1147BD+55 8242338324215 03 47 32.2+55 55 216.10 B9Vnn
HR 1148γBD+70 259234015006138W 03 50 21.5+71 19 564.63 A2IVn 3.9106.3
HR 1155BD+65 3692347512916I BE Cam03 49 31.2+65 31 344.47 M2+IIab eC:Large infrared excess.,G:In reflection nebula.,S:Ultraviolet FeII emission.,VAR:Lc 4.35 - 4.48V, amp. 0.12p.
HR 1158BD+62 6122352312917 03 49 36.7+63 17 505.85 A5Vn
HR 1161BD+56 8462359424244W 03 49 19.6+57 07 056.46 A0Vn 0.858.3
HR 1166BD+68 2862366212929 03 51 41.8+68 30 276.32 B9IVp
HR 1192BD+57 75224141242761105 03 53 43.3+57 58 305.80 A5m
HR 1196BD+71 2222416450402277 03 56 30.2+71 49 186.34 A5m
HR 1204BD+62 62824479129692281 03 57 25.5+63 04 205.03 B9.5V e
HR 1205BD+60 7682448012968I2867 03 57 08.3+61 06 325.00 K3I-II+A3V: 3.21.7D:Companion A0, CPM.,DYN:0.003".
HR 1241BD+68 30325274130062291I 04 06 03.1+68 40 485.87 K2III
HR 1242BD+58 69025291243842290 04 04 27.2+59 09 205.06 F0II
HR 1248BD+65 3912542513015 04 06 39.0+65 31 156.17 A3m
HR 1255BD+53 7322560224411 04 06 36.6+54 00 316.31 K0III-IV
HR 1260BD+61 67625638130312984 ASZ Cam04 07 51.1+62 19 486.99 B0III 0.317.9D:AB fixed. Some confusion in literature as to which component is A, which B. SZ CAM is Np = B, 6.94V, +0.41(B-V),,D:-0.53(U-B), O9.5V, vsini 160:k/s. Colors of both components have been described as "yellowish" even though both have,D:B-type spectra. Component Q, 10.39V, +0.58(B-V), -0.26(U-B).,G:Open cluster NGC 1502 #1, near center and probable member of cluster.,S:Luminosity of A variously classified II-III, V. Component B classified O9.5V, B0III or B0IIn.,SB:ADS 2984B, same period as for variable light. K 110.9k/s, V0 -22.8, asini 4.11.,VAR:Two variables: ADS 2984A = NSV 1458, amp. 0.05V, SB; component B = SZ Cam, Np, EA 7.0 - 7.29B, changing period, abrupt,VAR:change in 1972 from 2.6984378 to 2.69854365, later to 2.6985439d.
HR 1270BD+59 7592587724436 04 09 27.6+59 54 296.28 G8IIa
HR 1276BD+54 7402594824440 04 09 22.4+54 49 446.18 R F5V
HR 1281BD+71 239260765125 04 13 44.9+72 07 356.03 K1III
HR 1282BD+68 3102610113061 04 12 51.6+68 30 066.32 K0
HR 1296BD+57 78526553244952304 Var?04 15 01.8+57 27 376.08 A4III VAR:Probably var., amp. 0.08V.
HR 1305BD+61 6872667013075 04 16 53.6+61 51 015.70 B5Vn
HR 1313BD+57 7872675524514 04 17 08.2+57 51 385.71 K1III
HR 1314BD+53 75026764245122310 04 16 43.1+53 36 435.19 A2Vn
HR 1327BD+64 43327022130982315 04 20 40.3+65 08 265.27 G5IIb G:In Ursa cluster; Sirius group; UMa stream.
HR 1335BD+60 80027245131132317I 1558 04 21 47.6+60 44 085.39 M0III
HR 1342BD+56 9052732224563 04 21 51.8+56 30 245.88 R A3V
HR 1352BD+59 79327402245773146 1566 04 22 57.9+59 36 596.19 A4V 3.132.3VAR:ADS 3146B, 10.5 - >12V.
HR 1382BD+57 800278552461523243203 04 27 00.9+57 35 076.32 A0III 5.920.6D:Optical.
HR 1401BD+72 22728204523823333267 04 33 30.7+72 31 435.94 A8m 6.626.0G:Hyades group.,SB:4.195d, K 31.3k/s, V0 +9.0k/s, asini 1.81.
HR 14171BD+53 77928446246721653274 AVar?04 32 01.8+53 54 395.77 B0III 1.110.3D:AB binary. B, 6.94V, +0.16(B-V), -0.70(U-B), B1IV? vsini =<25k/s.,G:Cam OB1.
HR 1440BD+63 51528780131962336 04 36 24.2+64 15 425.94 A1V
HR 14662BD+53 79429316247443358 04 39 58.1+53 28 235.35 A8V 1.60.3D:AB 5.8 F0V, 7.4 F9V, 26.25y, a = 0.18" or 26.797y, a = 0.157". ABxC 5.6, 7.3, 425.0y, a = 1.38". Component D, 13.2v at,D:at 24" optical. Spectral classes component A, A9V; B, F8V; C, F8V.,DYN:0.004".
HR 14673BD+52 8652931724743I3359 1681 04 39 54.7+53 04 475.05 K0III 7.03.8SB:121d, K 28.2k/s, V0 -40.5k/s, asini 46.9.,VAR:ADS 3359A, Cep?, 5.05 - 5.10V, 5d?
HR 1468BD+76 174293295289 04 46 00.3+76 36 406.49 F7V
HR 1486BD+59 82629606247773391 04 43 18.1+59 31 156.50 R A7IV 0.00.1D:280.0y, e 0.56, a 0.45", i 51.9d, mag. diff 0.0.
HR 1491BD+75 189296785309173W 04 48 50.3+75 56 286.06 A9IV 6.096.9
HR 1510BD+70 3223008553262358 04 50 36.4+70 56 306.37 A0IV
HR 15114BD+56 97330121248291753432 04 48 00.3+56 45 265.30 A3m 7.599.0G:Hyades group.,S:Also classified A8IVbmvs.
HR 1515BD+55 9283014424834 04 48 07.0+55 36 096.26 R F0 G:Hyades group.
HR 1527BD+63 54330442132912362IW 04 52 05.2+63 30 195.44 M3IIIab 4.5115.4G:Eta Cep group.
HR 1542α9BD+66 3583061413298178 04 54 03.0+66 20 344.29 O9.5Ia eC:Color excess E(B-V) = +0.32.,G:In cluster NGC 1502. A possible runaway star from Cam OB1; in reflection nebula. Member assoc. Cam R1 at 870 pc.,S:H alpha emission due to extended envelope. uv 1548 absorption strong, 1394 very strong. Central Balmer emission in,S:blue-violet only.
HR 1546BD+52 8913075224894 04 53 09.8+52 50 276.41 A2V
HR 15555BD+55 941309582490423673508 04 55 03.1+55 15 335.52 B9.5V 6.412.9D:CPM.
HR 1561BD+52 8983113424919 04 56 07.1+52 52 105.75 A2V s
HR 15687BD+53 82931278249293536 04 57 17.2+53 45 084.47 A1V 3.40.4D:AB 4.5, 7.8, 284.0y, a = 0.78". C, 11v at 26" CPM, possibly physical.,G:UMa stream.,SB:ADS 3536A, 3.8845d, K 35.8k/s, V0 -9.5k/s, asini 1.91.
HR 1572BD+74 229313125385I 05 02 20.1+74 16 096.06 K5III
HR 1587BD+73 264315635403I 05 04 13.0+73 45 506.66 R K0
HR 15888BD+52 9063157924943I 04 59 46.3+53 09 206.08 K4III
HR 1589BD+73 265315905407W 05 04 39.8+74 04 015.96 R A1V 1.00.6D:136.0y, e 0.32, a 0.425", i 88d, mag. diff 1.0.
HR 1593BD+60 85331662133413590 05 01 35.9+61 04 416.03 F4V 5.55.4D:CPM.
HR 1594BD+66 3703167513344 05 02 50.4+66 49 226.19 dF6 G:Hyades group.
HR 1603β10BD+60 8563191013351182I3615 A05 03 25.1+60 26 324.03 G1Ib-IIa 3.480.8C:Color excess E(B-V) = +0.16.,G:Group with HR 1622 and 1719, all nearly same proper motion.
HR 162211BD+58 8043234325001W BV Cam05 06 08.5+58 58 215.08 B2.5Ve 1.0180.5D:Optical pair with HR 1623.,G:Group with HR 1603, 1719.,RV:Pole on. Rotationally unstable Be shell star.,VAR:Gamma Cas, amp. 0.07V, period a few hours?
HR 162312BD+58 8053235725003W BM Cam05 06 12.2+59 01 166.08 K0III 1.0180.5D:Optical pair with HR 1622; C, 10.8v at 173" from B; D, 13.3 at 16" from B.,SB:80.1745d, K 22.7k/s, V0 +0.6k/s, asini 23.4.,VAR:RS CVn amp. 0.14V, 82.8d.
HR 1624BD+60 8573235613369I 05 06 29.7+61 10 126.04 K5II
HR 1630BD+54 85932445250073667 05 06 22.0+54 24 217.24 R G5 3.76.7M:HR mag. 6.31 should have been 7.31.
HR 1636BD+69 30232518133822382 05 09 36.7+69 38 226.41 K1III
HR 1643BD+73 2743265054552387 BN Cam05 12 22.4+73 56 485.43 B9pSi RV:At times variable in period 7.993d.,VAR:Alpha CV, amp. 0.10U, 0.06B, 0.05V, 0.7325d.
HR 1647BD+64 50032715133882384 05 09 44.5+64 55 106.41 F6V
HR 1650BD+76 1903278154643738 1854 05 14 35.6+76 28 226.37 A0V 4.51.5VAR:ADS 3738B, amp. 1.8v?
HR 1675BD+61 7663326613409 05 13 03.2+61 51 006.17 A2III
HR 167814BD+62 7343329613413 05 13 31.3+62 41 296.50 A7Vn
HR 1683BD+73 280335415483 05 18 13.3+73 16 055.74 R A0V
HR 1686BD+79 1693356454961913864 A05 22 33.5+79 13 525.05 F6V 3.710.4D:B, dF5, optical. C observed only once.
HR 1688BD+59 8573361825088 05 15 11.3+59 24 206.15 K2III-IV
HR 171915BD+57 8743423325125 05 19 27.8+58 07 026.13 B5V G:Group with HR 1603, 1622. Cas-Tau OB1.
HR 1720BD+62 74234255134602397I 05 20 22.6+62 39 135.61 K4I:
HR 1745BD+77 1953465355352404 05 29 25.7+77 58 396.56 A7III
HR 175116BD+57 87934787251612402W 05 23 27.8+57 32 405.28 A0Vn 7.7106.2
HR 180217BD+62 7593558313518203I 2003 05 30 10.2+63 04 025.42 M1IIIa
HR 182818BD+57 88936066252411150 2058 05 32 33.8+57 13 166.48 F8V
HR 1844BD+74 252363845593205I 2337 05 39 43.7+75 02 386.17 M0III
HR 1853BD+66 4013649613548W 05 37 16.2+66 41 466.26 A8Vn 0.80.3
HR 185719BD+64 53636570135504177 05 37 15.1+64 09 176.15 A0V 4.01.6D:CPM.
HR 1916BD+65 48537289135702426I 05 42 26.4+65 41 525.60 gK5
HR 194124BD+56 10503760125333 05 43 01.6+56 34 546.05 K0III
HR 194323BD+61 8163763813590 05 44 08.6+61 28 366.15 gG5
HR 196926BD+56 10583809125362 2615 05 46 30.4+56 06 565.94 A4Vn
HR 1976BD+62 78438284136184376 05 49 04.9+62 48 296.13 R A4V 0.90.9
HR 199229BD+56 106538618254034412 05 50 34.0+56 55 086.54 A4IV-V 4.225.1D:Third component mag. diff 6.29V, 80" from A.
HR 1994BD+68 41238645136352438 05 52 55.5+68 28 176.20 G9III
HR 200630BD+58 8633883125419 05 52 17.4+58 57 516.14 A0V s
HR 202731BD+59 92039220254472446 TU Cam05 54 57.8+59 53 185.20 A2V SB:2.9333d, K 78.0k/s, V0 -4.0k/s, asini 3.15.,VAR:EB 5.12 - 5.29V, 2.933241d.
HR 2041BD+66 41339429136622448 05 57 35.0+66 05 466.25 K0
HR 2078BD+75 2474005557302459 06 05 09.3+75 35 096.40 R K5
HR 2121BD+59 9374082725551 06 05 08.3+59 23 356.34 K1III-IV G:Probable Hyades group.
HR 2126BD+63 6304095613715 06 06 39.2+63 27 136.39 R K0
HR 215237BD+58 8974159725597I 06 09 59.1+58 56 095.36 G8III
HR 216536BD+65 5174192713756233I 06 12 51.1+65 43 065.32 K1.5IIIbCN-0.5
HR 220140BD+60 9384263313772IW 06 15 40.6+59 59 575.35 K3III 5.1102.7
HR 2209BD+69 3714281813788234 06 18 50.8+69 19 114.80 A0Vn
HR 2285BD+70 4014447258615039 06 28 14.6+70 32 085.97 R A4V 5.95.7D:CPM.
HR 2346BD+79 208455605911 06 40 16.8+79 35 586.54 R A1V
HR 2350BD+82 1774561810433950 06 44 30.2+82 06 556.65 A5V
HR 2363BD+78 2274586659192507I 06 40 28.8+77 59 455.73 gK5
HR 2365BD+73 3404594759092503 06 37 54.9+73 41 446.24 F2
HR 2396BD+71 3594650959252511 06 40 32.2+71 44 565.92 K0III
HR 2401BD+79 212465885946248 06 46 14.1+79 33 535.45 F8V SB:60.0d, K 1.7k/s, V0 +16.2k/s, asini 1.245. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,SB:Unresolved by speckle interferometry.
HR 249042BD+67 45448879139732523 06 50 57.1+67 34 195.14 B4IV
HR 251143BD+69 3944934013986259 06 53 42.2+68 53 185.12 B7III
HR 2527BD+77 266498786022260I 07 00 04.0+76 58 394.55 K4III G:Wolf 630 group.
HR 2581BD+70 430508856041IW 07 01 21.5+70 48 295.68 gK4 5.3117.0
HR 2617BD+70 432520306074I 07 05 51.8+70 43 556.50 R K0III
HR 2681BD+72 3525407061152552 07 13 58.1+71 49 006.35 K0
HR 2709BD+81 242550751164 07 25 21.9+81 15 276.31 A0III
HR 2742BD+82 2015596611793951I VZ Cam07 31 04.4+82 24 414.96 M4IIIa G:Hyades group.,VAR:SR 4.80 - 4.96V, 6.40 - 6.70p, 23.7d.
HR 277247BD+60 104856820262985995 07 22 17.2+59 54 076.35 A8m 4.52.2
HR 2797BD+81 252575081194 07 34 39.7+80 53 486.41 R gG7
HR 2809BD+66 50257742141952571 07 27 25.8+66 19 546.47 B9III
HR 2830BD+68 4805842514211284I 07 30 52.7+68 27 565.64 gK2
HR 297551BD+65 59362066143212602 07 46 40.1+65 27 215.92 gK2
HR 297749BD+63 7336214014322 BC Cam07 46 27.4+62 49 506.49 F0pSrEu VAR:Alpha CV 6.43 - 6.48V, 4.285d. Magnetic field same period.
HR 2997BD+80 238626131254 07 56 17.3+80 15 566.56 G8V
HR 3075BD+74 338643076378300I 08 00 11.7+73 55 055.41 K3III
HR 3082BD+79 2656448663922617W 08 04 47.1+79 28 475.42 A0pSi 8.36.7S:Magnetic star.
HR 3108BD+84 1696529913001639 08 16 53.8+84 03 286.49 A3IV
HR 310953BD+60 11056533914402302S AX Cam08 01 42.4+60 19 286.01 A2pSrCrEu vRV:1.14229d, 8d, and order of years. Possibly binary.,SB:2380d, K about 8k/s, V0 -2.2k/s, asini 220.,VAR:Alpha CV 5.95 - 6.08V, 8.0278d. 1.14d also possible. Length of period varies in cycles 1.8 yrs. Magnetic and,VAR:spectrum variable 8.0269d; also rotation period.
HR 3112BD+63 74965448144072619W 08 02 30.8+63 05 256.40 G1III 2.448.6
HR 3197BD+82 2356793413193952 08 24 32.9+82 25 516.32 A2Vn
HR 3216BD+76 310683756487310 08 19 32.2+75 45 255.54 G8III
HR 3352BD+75 3427197365926872 4133 08 36 48.7+74 43 256.31 A2m 3.51.8D:CPM.,SB:ADS 6872A, 4.285d, K 63.5k/s, V0 -7.4k/s, asini 3.72.,VAR:ADS 6872B, L 9.0 - >12v.
HR 3379BD+74 370725826605322 08 39 42.6+73 37 476.15 G7III
HR 3581BD+84 1967699014611640 09 15 21.2+84 10 526.33 F2III
HR 3666BD+74 393795176816 09 19 55.8+74 00 596.50 R G8III
HR 3934BD+84 2258632116373955 Var10 08 34.3+83 55 066.37 K0 VAR:Amp. 0.13V.
HR 4062BD+84 234895711701 10 29 41.5+84 15 085.50 F0IV G:Hyades group.
HR 4084BD+83 297900891714911 4864 10 31 04.6+82 33 315.26 F2V
HR 4429BD+81 3739994518843956 5230 11 31 50.4+81 07 386.15 A2m
HR 4586BD+81 38910421619673957I 5415 12 00 18.6+80 51 116.17 M2III G:61 Cyg group.
HR 4606BD+86 17610490419751642 12 04 28.1+85 35 146.27 F6V
HR 4609BD+77 4611049857500451 12 05 15.1+76 54 215.80 G9III
HR 4639BD+82 3561059431991W 12 11 00.0+81 42 366.00 gK5 2.066.7
HR 4646BD+78 4121061127522454 12 12 11.9+77 36 595.14 A5m SB:1.2710d, K 63.2?k/s, V0 +0.3k/s, asini 1.10.
HR 4852BD+81 40211111220803017 12 44 26.0+80 37 166.40 A5m S:Also classified A5V, A6III.
HR 4892BD+84 28911201421018682 B12 49 06.6+83 25 055.85 A0V+A2V 0.521.6D:CPM with HR 4893.,N:With HR 4893 called 32 Cam in Hevelius and some later catalogues. NOT Flamsteed 32. In BAC the two are listed as in UMi.,N:Fl. 32 Cam = 30 Aur = HR 2029.,SB:ADS 8682B, 3.2866d, K 108.3k/s, V0 -0.1k/s, msin3i 2.47, asini 4.89. vsini both components 17k/s.
HR 4893BD+84 29011202821028682 A12 49 13.6+83 24 465.28 A1IIIShell 0.521.6D:CPM with HR 4892.,N:See HR 4892.
HR 5009BD+81 41611533721643056W 6153 13 12 25.4+80 28 176.25 K0Ib 4.01.1S:Also classified G8III + A8V:.,VAR:Fainter component 8.5 - 10.5v.
HR 5091BD+79 42211756678213075 13 26 56.7+78 38 385.77 G2.5IIIbCH1
HR 5131BD+77 5161186867848I 13 34 42.8+76 32 486.57 R K5III:
HR 5203BD+83 39712056522661643 13 42 23.1+82 45 095.98 G9III

Legend

Key to columns [154]
HRHarvard Revised Number = Bright Star Number
BBayer designation (greek letter)
FFlamsteed number
DMDurchmusterung Identification (BD = Bonn; CD = Cordoba; CP = Cape Photographic)
HDHenry Draper Catalog Number
SAOSAO Catalog Number
FK5FK5 star Number
IRI 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;)
ADSAitken's Double Star Catalog (ADS) designation
VarIDVariable star identification
RARight Ascension (J2000.0)
DecDeclination (J2000.0)
vMagVisual magnitude
spTypeSpectral type
dMagMagnitude difference of double, or brightest multiple
SepSeparation of components in Dmag if occultation binary (arcsec)
RemarksNote 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