1994A&A...292..115A


Query : 1994A&A...292..115A

1994A&A...292..115A - Astronomy and Astrophysics, volume 292115-118 (1994/12-1)

Dynamics of nearby multiple stars. The α Centauri system.

ANOSOVA J., ORLOV V.V. and PAVLOVA N.A.

Abstract (from CDS):

The triple star system α Cen AB and Proxima Cen - the component C - is the nearest to the Sun. The study of its dynamics has shown that this system is probably not a chance one. The motion of the component C (Proxima) with respect to the centre of mass of the pair AB is hyperbolic with the probability P=1.0. We observe, therefore, a slow passage of C close to the pair AB. We propose the hypothesis that this system is a part of a stellar moving group. We list the probable members of this group amongst the nearby stars. Amongst them we have the binaries Gliese 140.1 and 676, the triple system ADS 10288 (Gliese 649.1), and six single stars. The probability to find these stars by chance inside the velocity space cube with a side of 20km/s around α Cen is equal to about 2%.

Abstract Copyright: ∼

Journal keyword(s): binaries: general - stars: individual: α Cen - stellar dynamics - solar neighbourhood

Nomenclature: Table 9: [AOP94] NN N=11

Simbad objects: 20

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Number of rows : 20
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HD 38 ** 00 05 41.01985 +45 48 43.5072 10.86 9.645 8.217 8.30   K6V+M0.5V 93 0
2 * tet Scl PM* 00 11 44.0210769384 -35 07 59.212953084   5.661 5.239     F5V 161 0
3 HD 1273 SB* 00 16 53.8974209976 -52 39 04.166413161 7.537 7.497 6.852 6.475 6.095 G5VFe-1.2CH-0.9 97 0
4 HD 4391 EB* 00 45 45.5929295136 -47 33 07.142647212   6.418 5.794     G3V 135 0
5 HD 17948 PM* 02 55 56.9208409368 +61 31 16.094508276   6.001 5.584     F5V 101 0
6 HD 21209B PM* 03 23 15.8895353604 -49 59 38.743504037   11.71 10.32 9.925   K8Vk: 48 0
7 HD 21209 PM* 03 23 17.1766583819 -49 59 30.913415913   9.67 8.59     K3.5V 87 0
8 1RXS J032315.8-495940 ** 03 23 17.18 -49 59 30.9           ~ 3 0
9 NAME Proxima Centauri PM* 14 29 42.9461331854 -62 40 46.164680672 14.21 12.95 11.13 9.45 7.41 M5.5Ve 1483 0
10 * alf Cen B PM* 14 39 35.06311 -60 50 15.0992 2.89 2.21 1.33     K1V 1092 2
11 * alf Cen A SB* 14 39 36.49400 -60 50 02.3737 0.96 0.72 0.01     G2V 1352 1
12 * alf Cen ** 14 39 36.50 -60 50 02.3   0.4 -0.1     G2V+K1V 1031 0
13 * ksi Sco ** 16 04 22.134576 -11 22 23.17404 4.65 4.64 4.17     F7V 134 0
14 * gam02 Nor PM* 16 19 50.4223079953 -50 09 19.821590813 6.27 5.10 4.02 3.24 2.66 K0III 78 0
15 HD 153525 BY* 16 57 42.2279930304 +47 21 43.714092384       7.3   K3V 116 0
16 HD 153557 BY* 16 57 53.1786346617 +47 22 00.062086057   8.80 7.82 8.49   K3V 121 0
17 HD 153557B PM* 16 57 53.6142932703 +47 22 02.442948894   12.086   10.1   M1.5V 47 0
18 CD-51 10924 PM* 17 30 11.2044753442 -51 38 13.130309109 12.317 11.028 9.585 8.675 8.60 M0V 142 1
19 CD-51 10924B PM* 17 30 16.2379465451 -51 38 22.595533702   15.05 13.37 13.03 10.49 M3V 28 0
20 HD 175225 PM* 18 51 34.9201379040 +52 58 30.246268944   6.35 5.52     G9IVa 123 0

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