2018RAA....18...94S


Query : 2018RAA....18...94S

2018RAA....18...94S - Research in Astron. and astroph., 18, 94-94 (2018/August-0)

Estimating masses of selected stars in the Pulkovo program by means of astrometry methods.

SHAKHT N.A., GORSHANOV D.L. and VASILKOVA O.O.

Abstract (from CDS):

Stars in the Pulkovo Observatory program are observed with a 65-cm refractor during many years to study their positions and movements. We present examples of two visual binary stars, for which orbits and masses of components were determined, and two astrometric stars, for which masses of their unseen companions were estimated. The first two stars are ADS 14636 (61 Cygni) and ADS 7251, and the others are Gliese 623 and ADS 8035 (Alpha UMa). Direct astrometric methods are used for estimation of mass-ratio and masses.

Abstract Copyright:

Journal keyword(s): stellar masses - orbits - binaries: individual: ((61 Cygni, Alpha UMa, Gliese 623, ADS 7251))

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 HD 79210 SB* 09 14 22.7748624830 +52 41 11.791503353   9.388   6.8   K7V 310 0
2 HD 79211 Er* 09 14 24.6828466599 +52 41 10.902471910   7.966   6.8   M0V 301 0
3 * alf UMa B PM* 11 03 43.598848 +61 45 03.14311   5.26 4.86     A7.5 5 0
4 * alf UMa A PM* 11 03 43.668632 +61 45 03.72003   3.01 1.87     G9III 11 0
5 * alf UMa SB* 11 03 43.67152 +61 45 03.7249 3.78 2.86 1.79 0.98 0.40 G9III+A7.5 439 0
6 G 202-45 SB* 16 24 09.3137145795 +48 21 11.107573476   12.099       M3.0V 182 1
7 [EG97] S1 * 17 45 40.0418 -29 00 28.324           B0/2V 93 0
8 * 61 Cyg A BY* 21 06 53.9395895022 +38 44 57.902349973 7.50 6.39 5.21 4.19 3.54 K5V 1036 0
9 * 61 Cyg ** 21 06 53.95 +38 44 57.9           ~ 177 0
10 * 61 Cyg B Er* 21 06 55.2638444466 +38 44 31.358519864 8.63 7.40 6.03 4.86 3.55 K7V 722 0

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