EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 507 / No 1 (November III 2009) A&A, 507 1 (2009) 251-259 Full HTML
Free Access

   

Table A.1:

Basic data from the literature of Washington double stars with tabulated angular separations $\rho > 1000$ arcsec.

WDS 		Discovery Simbad $\alpha $ $\delta$ $\mu_\alpha \cos{\delta}$ $\mu_\delta$ $d_\pi$ Vb J $K_{\rm s}$ Sp. $\rho $ $\theta$
identifier designationa name (J2000) (J2000) [mas a-1] [mas a-1] [pc] [mag] [mag] [mag] type [arcsec] [deg]
00059+1805 LEP 1AE HD 101 00 05 54.74 +18 14 05.8 - $152.2\pm 1.1$ - $148.1 \pm 1.4$ $37.1\pm0.8 $ 7.46 $6.332\pm0.019$ $6.034\pm0.024$ F8 1606.8 245.9
    LP 404-21 00 04 11.81 +18 03 10.7 -146 -146 ... 16.3 $14.068\pm0.030$ $13.339\pm0.029$ ...    
00152+2454 GIC 4 G 131-46 00 16 53.59 +24 20 48.7 -$136\pm11$ -$204\pm10$ ... 13.6 $9.944\pm0.020$ $9.067\pm0.017$ K 2469.8 145.8
    G 130-59 00 15 11.85 +24 54 52.1 -$105\pm11$ -$215\pm11$ ... 14.5 $12.600\pm0.022$ $11.951\pm0.022$ ...    
00400-1533 LDS 5286 LP 765-52 00 37 29.44 -15 45 52.3 $+173\pm5 $ -$19\pm5$ ... 15.5 * $11.890\pm0.021$ $11.038\pm0.023$ ... 2274.9 71.5
    LP 765-57 00 39 59.21 -15 34 07.9 $+169\pm5 $ -$34\pm5$ ... 15.2 * $13.317\pm0.026$ $12.746\pm0.035$ ...    
00435+3351 WEI 46AC GJ 30 00 43 32.90 +33 50 41.3 - $204.0\pm0.8 $ - $357.2\pm0.6$ $20.6\pm0.4 $ 8.73 $6.592\pm0.018$ $5.938\pm0.016$ K8 1295.0 266.8
    BD+33 96 00 41 49.11 +33 51 54.8 $+8.3\pm1.2 $ $+1.8\pm1.2$ ... 8.63 $6.639\pm0.021$ $5.966\pm0.018$ K0    
00520+2035 GIC 16 G 69-27 00 52 00.03 +20 34 58.6 $+176.5\pm1.8 $ - $107.4\pm1.5$ $32\pm3 $ 11.40 $8.490\pm0.019$ $7.628\pm0.020$ ... 1614.0 56.1
    G 69-29 00 53 35.48 +20 49 59.4 $+213\pm11 $ -$132\pm11$ ... 13.9 * $10.095\pm0.021$ $9.248\pm0.015$ ...    
01024+0504 WNO 50AC HD 6101 AB 01 02 24.60 +05 03 41.4 $+323.3\pm1.2 $ $+226.0\pm1.2$ $21.1\pm0.5 $ 8.16 $6.199\pm0.019$ $5.510\pm0.020$ K2+... 1276.0 87.8
    G 1-45 AB 01 03 49.94 +05 04 30.7 $+317\pm8 $ $+227\pm8$ $21.3\pm1.7 $ 14.10 $13.504\pm0.024$ $13.418\pm0.034$ DA5    
01163-3217 LDS 1091 LP 883-336 01 16 21.75 -31 58 12.2 $+408\pm5 $ -$1\pm5 $ ... 17.9 * $11.899\pm0.022$ $11.001\pm0.023$ ... 1151.0 186.0
    LP 883-337 01 16 12.35 -32 17 17.0 $+388\pm5 $ $+17\pm5 $ ... 18.0 * $13.884\pm0.026$ $13.132\pm0.034$ ...    
02255-0904 GRV 1148 WD 0223-092 02 25 30.96 -09 04 14.9 $+81\pm5 $ -$2\pm5 $ ... 19.5 * ... ... DA4.6 1272.1 228.2
    WD 0221-095 02 24 26.96 -09 18 23.5 $+85\pm4 $ -$0\pm4 $ ... 19.8 * ... ... DA5.8    
02310+0823 GIC 32 G 73-63 02 31 03.28 +08 22 55.1 $+376.1\pm1.9 $ - $85.4\pm1.6$ $33\pm3 $ 10.90 $8.356\pm0.023$ $7.554\pm0.023$ K4-7V: 3094.6 277.9
    G 73-59 02 27 36.68 +08 29 58.8 +350 -63 ... 16.1 * $11.271\pm0.026$ $10.455\pm0.021$ ...    
03162+5810 LEP 13AC GJ 130.1 A 03 16 13.82 +58 10 02.4 $+445.6\pm3.9 $  -$340.3\pm4.1$ $14.4\pm0.7 $ 10.53 $7.344\pm0.020$ $6.566\pm0.024$ M2 1164.1 197.6
    G 246-30 03 15 29.44 +57 51 33.0 +467 -237 ... 15.5 * $11.121\pm0.024$ $10.271\pm0.019$ M:    
03330+0306 LDS 3504 G 80-8 03 32 59.02 +03 06 08.0 +294.8 -80.9 ... 13.1 * $10.102\pm0.023$ $9.281\pm0.023$ ... 429.5 266.4
    NLTT 11184 03 32 30.40 +03 05 40.8 +286 -77 ... 17.0 * $12.491\pm0.026$ $11.750\pm0.029$ ...    
03442-6448 LDS 104 $\beta$ Ret AB 03 44 11.96 -64 48 24.9 $+310.1\pm0.7 $ $+83.2\pm0.6 $ $29.9\pm0.5 $ 3.84 $1.937\pm0.310$ $1.279\pm0.270$ K2III SB 1466.3 94.2
    HD 24293 03 48 01.12 -64 50 11.7 $+334.0\pm1.0 $ $+99.0\pm1.1 $ $40.5\pm1.3 $ 7.85 $6.630\pm0.029$ $6.241\pm0.024$ G3V    
07590-6338 LDS 199 CD-63 370 07 58 57.36 -63 37 45.5 - $143.0\pm1.7 $ $+262.5\pm1.8$ ... 9.90 $8.826\pm0.034$ $8.502\pm0.023$ F8 1033.4 195.8
    L 137-85 07 58 14.99 -63 54 19.6 -$178\pm10 $ $+384\pm10$ ... 11.2 * $9.791\pm0.024$ $9.175\pm0.023$ ...    
10197+1928 WNO 53 40 Leo 10 19 44.20 +19 28 15.8 - $230.0\pm0.9 $ - $214.7\pm0.5$ $21.37\pm0.11 $ 4.78 $4.037\pm0.292$ $4.020\pm0.314$ F6IV 5231.4 308.3
    LP 371-59 A 10 14 53.94 +20 22 18.9 -225 -198 ... 15.3 * $10.815\pm0.026$ $9.99\pm0.023$ M5    
11125+3549 STTA 108BD HD 97371 11 12 44.28 +35 49 48.4 - $60.1\pm0.7 $ -$7.8\pm0.7 $ $141\pm13 $ 7.20 $5.423\pm0.019$ $4.805\pm0.018$ K0 2100.8 88.5
    HD 97832 11 15 36.98 +35 50 44.7 $+0.1\pm1.2$ -2.2$\pm$1.3 ... 8.20 $6.668\pm0.021$ $6.194\pm0.018$ G5    
11452+1821 GIC 101 G 57-17 11 45 11.92 +18 20 58.7 -$296\pm8$ -$296\pm8$ ... 13.27 $9.162\pm0.022$ $8.260 \pm 0.016$ M4 1341.3 280.2
    G 57-15 11 43 39.18 +18 24 56.9 -259 -267 ... 15.07 $12.863\pm0.026$ $12.097\pm0.021$ ...    
11455+4740 LEP 45 HD 102158 11 45 30.58 +47 40 01.1 -591.6 $\pm$ 0.7 -290.7 $\pm$ 0.5 49.3 $\pm$ 1.7 8.06 6.860 $\pm$ 0.026 6.509 $\pm$ 0.026 G2V 1176.1 72.4
    G 122-46 11 47 21.66 +47 45 56.7 -585 -200 ... 14.16 10.586 $\pm$ 0.020 9.846 $\pm$ 0.020 M:    
13090+3353 LEP 62AC LP 268-35 13 08 58.26 +33 53 10.0 -209.7 $\pm$ 2.3 -111.8 $\pm$ 1.7 66 $\pm$ 12 11.56 9.296 $\pm$ 0.019 8.623 $\pm$ 0.018 ... 1273.8 192.3
    LP 268-33 13 08 36.42 +33 32 25.7 -208.8 $\pm$ 5.5 -101.2$~\pm~$5.5 ... 16.3 * 11.685 $\pm$ 0.021 10.769 $\pm$ 0.019 ...    
13410+6808 LDS 5788 G 238-50 13 44 29.36 +68 27 50.3 -269.9 $\pm$ 1.5 +43.5 $\pm$ 1.8 40 $\pm$ 3 11.17 8.845 $\pm$ 0.021 8.023 $\pm$ 0.015 M2 1696.8 44.5
    LP 40-200 13 40 54.27 +68 07 43.8 -265.5 $\pm$ 1.8 +32.8 $\pm$ 1.8 ... 11.83 9.837 $\pm$ 0.019 9.138 $\pm$ 0.020 K3    
13599+2520 BUP 156 BD+26 2517 AB 14 01 11.60 +25 21 36.2 +5.5 $\pm$ 1.4 +36.2 $\pm$ 1.3 ... 9.51 8.337 $\pm$ 0.023 8.060 $\pm$ 0.018 G0 1033.9 83.2
    BD+26 2513 13 59 55.87 +25 19 33.7 $+20.5\pm1.2$ -55.9 $\pm$ 1.2 ... 10.41 9.433 $\pm$ 0.021 9.145 $\pm$ 0.019 F8    
14396-6050c LDS 494AC $\alpha $ Cen AB 14 39 35.93 -60 50 07.0 -3633.7 $\pm$ 0.7 +702.3 $\pm$ 0.6 1.325 $\pm$ 0.007 1.35 -1.454 $\pm$ 0.133 -2.008 $\pm$ 0.260 G2V+K1V 7860.1 236.9
    Proxima 14 29 42.91 -62 40 46.5 -3775.8 $\pm$ 1.6 +766 $\pm$ 2 1.296 $\pm$ 0.004 11.01 5.357 $\pm$ 0.023 4.384 $\pm$ 0.033 M5.5Ve    
15208+3129 LEP 74 HD 136654 15 20 50.07 +31 28 48.5 -180.0 $\pm$ 0.4 +139.0 $\pm$ 0.5 43.5 $\pm$ 1.1 6.90 5.982 $\pm$ 0.020 5.742 $\pm$ 0.027 F5V 1580.6 325.6
    BD+32 2572 15 19 40.15 +31 50 32.9 -181.2 $\pm$ 0.6 +140.2 $\pm$ 0.8 42 $\pm$ 2 9.03 7.569 $\pm$ 0.021 7.115 $\pm$ 0.020 K0V    
16348-0412 GIC 144AB HD 149414 AB 16 34 42.36 -04 13 44.1 -133.7 $\pm$ 1.4 -701.2 $\pm$ 1.4 45 $\pm$ 3 9.60 8.055 $\pm$ 0.024 7.517 $\pm$ 0.024 G5Ve SB1 1176.5 36.4
    BD-03 3968B 16 35 29.03 -03 57 57.2 -162 -685 ... 13.86 11.086 $\pm$ 0.022 10.541 $\pm$ 0.022 M:    
18111+3241 LEP 87 BD+32 3065 18 11 06.22 +32 41 00.3 -134.7 $\pm$ 1.2 +322.1 $\pm$ 1.3 46 $\pm$ 3 10.52 8.590 $\pm$ 0.039 7.931 $\pm$ 0.020 K5 1106.0 148.3
    G 206-16 18 11 52.28 +32 25 20.0 -143 +318 ... 15.6 * 10.885 $\pm$ 0.021 10.024 $\pm$ 0.017 ...    
20084+1503 LDS 1033AF G 143-33 20 08 21.93 +15 02 36.6 -159.1 $\pm$ 1.7 -180.7 $\pm$ 1.7 ... 11.56 9.408 $\pm$ 0.028 8.409 $\pm$ 0.024 ... 2186.6 269.0
    G 143-27 20 05 51.01 +15 01 59.2 -156 -210 ... 12.88 11.626 $\pm$ 0.022 11.245 $\pm$ 0.020 ...    
20124-1237 TDT 2085AC $\xi ^{02}$ Cap 20 12 25.86 -12 37 02.5 +193.4 $\pm$ 0.4 -196.0 $\pm$ 0.5 27.7 $\pm$ 0.3 5.84 4.971 $\pm$ 0.020 4.634 $\pm$ 0.017 F7V 1021.3 193.6
    LP 754-50 20 12 09.44 -12 53 35.1 +195.3 $\pm$ 2.0 -194.8 $\pm$ 1.8 23.6 $\pm$ 1.4 11.30 8.485 $\pm$ 0.023 7.625 $\pm$ 0.021 M0Vk    
20302+2651 BUP 213AE HD 340345 AB 20 30 10.67 +26 50 34.5 -145.9 $\pm$ 2.7 -141.9 $\pm$ 2.7 23.8 $\pm$ 1.8 9.69 7.133 $\pm$ 0.021 6.347 $\pm$ 0.020 M1V+ 1338.7 93.2
    HD 340459 20 31 50.53 +26 49 19.3 -8.1 $\pm$ 1.4 -5.5 $\pm$ 1.4 ... 10.15 8.235 $\pm$ 0.023 7.647 $\pm$ 0.016 G5    
20452-3120 LDS 720AB AU Mic 20 45 09.49 -31 20 26.7 +279.6 $\pm$ 1.2 -360.3 $\pm$ 0.8 9.92 $\pm$ 0.10 8.81 5.436 $\pm$ 0.017 4.529 $\pm$ 0.020 M1Ve 4680.9 212.8
    AT Mic AB 20 41 51.12 -32 26 07.3 +261.3 $\pm$ 3.6 -344.8 $\pm$ 3.9 10.7 $\pm$ 0.4 10.27 5.807 $\pm$ 0.026 4.944 $\pm$ 0.042 M4Ve+M5:    
20599+4016 LEP 98AD HD 200077 AE-D 20 59 55.24 +40 15 31.4 +230.5 $\pm$ 01.1 +211.2 $\pm$ 1.3 41.0 $\pm$ 0.9 6.58 5.450 $\pm$ 0.021 5.119 $\pm$ 0.024 F8+ 1212.8 258.5
    G 210-44 AB 20 58 11.48 +40 11 29.0 +229.7 $\pm$ 1.2 +202.9 $\pm$ 1.2 46 $\pm$ 4 10.75 8.142 $\pm$ 0.030 7.339 $\pm$ 0.018 M1    
22175+2335 GIC 179 G 127-13 22 17 25.87 +23 35 04.7 -104 $\pm$ 12 -388 $\pm$ 11 ... 14.1 * 9.890 $\pm$ 0.019 9.057 $\pm$ 0.023 ... 2107.7 12.7
    G 127-14 22 17 59.56 +24 09 21.1 -124 $\pm$ 10 -416 $\pm$ 10 ... 14.2 * 10.276 $\pm$ 0.021 9.49 $\pm$ 0.018 ...    
23228+2208 GIC 191 BD+21 4923 23 22 48.81 +22 07 59.4 +198.3 $\pm$ 1.2 -69.8 $\pm$ 1.2 71 $\pm$ 9 9.71 8.293 $\pm$ 0.020 7.851 $\pm$ 0.016 F5 3265.3 253.9
    G 68-7 23 19 03.21 +21 52 54.5 +310 $\pm$ 11 -101 $\pm$ 11 ... 14.7 * 11.589 $\pm$ 0.020 10.784 $\pm$ 0.018 ...    
a
References of discovery names - BUP: Burnham, S. W. proper motion stars (from additional ``DD'' list): GIC: Giclas et al. (1961); GRV: Greaves, J. private communication (from data in Eisenstein et al. 2006); LEP: Lépine & Bongiorno (2007); LDS: Luyten, W. J. proper motion catalogues (e.g. Luyten 1941); STF: Struve, F. J. W. (several citations by e.g.: Herschel 1833; Bessel 1833); STTA: Struve, O. ``DD'' (Appendix list); TDT: Tycho Double Star (from additional ``DD'' list); WNO: Washington Observations; WEI: Weisse, M. (cited in, e.g., Burnham Double Star Catalogue 1906).
b
 V-band magnitudes marked with an asterisk are estimated from four epochs of photographic BJ and RF magnitudes or from Sloan g and r magnitudes. Remaining V-band magnitudes are from the literature (see main text).
c
The proper motion of the primary in the system corresponds to $\alpha $ Cen A. The apparent difference with respect Proxima (of up to $292 \pm 4$ mas a-1 in $\mu_\delta$) is due to the strong dynamical effect on $\alpha $ Cen A by its close companion, $\alpha $ Cen B.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.