scholarly journals Detection of a white dwarf in a visual binary system

1992 ◽  
Vol 104 ◽  
pp. 1539 ◽  
Author(s):  
Erika Boehm-Vitense

1993 ◽  
Vol 137 ◽  
pp. 554-556
Author(s):  
Timothy M. Brown ◽  
Jørgen Christensen-Dalsgaard ◽  
Barbara W. Mihalas

AbstractPulsation frequency separations, combined with other observations, can constrain the structural parameters of Sun-like stars. As an example, we treat a hypothetical visual binary system resembling α Cen.



1995 ◽  
Vol 107 ◽  
pp. 219 ◽  
Author(s):  
S. M. Andrievsky ◽  
I. V. Chernyshova ◽  
I. A. Usenko ◽  
V. V. Kovtyukh ◽  
V. E. Panchuk ◽  
...  


1996 ◽  
Vol 281 (3) ◽  
pp. 1001-1015 ◽  
Author(s):  
R. D. Jeffries ◽  
D. A. H. Buckley ◽  
D. J. James ◽  
J. R. Stauffer






1985 ◽  
Vol 90 ◽  
pp. 346 ◽  
Author(s):  
R. L. Walker ◽  
C. R. Chambliss


2021 ◽  
Author(s):  
Suhail G. Masda ◽  
A. R. Khan ◽  
J. M. Pathan


Astrophysics ◽  
2018 ◽  
Vol 61 (4) ◽  
pp. 444-457 ◽  
Author(s):  
E. V. Polyakov ◽  
O. O. Vasilkova ◽  
D. L. Gorshanov ◽  
M. A. Pogodin ◽  
N. A. Shakht


1989 ◽  
Vol 114 ◽  
pp. 408-412
Author(s):  
Rex A. Saffer ◽  
James Liebert

AbstractWe report on a search for short-period binary systems composed of pairs of evolved stars. The search is being carried out concurrently with a program to characterize the kinematical properties of two different samples of stars. Each sample has produced one close binary candidate for which further spectroscopic observations are planned. We also recapitulate the discovery of a close detached binary system composed of two cool DA white dwarfs, and we discuss the null results of Hα observations of the suspected white dwarf/brown dwarf system G 29–38.



1999 ◽  
Vol 191 ◽  
pp. 437-446 ◽  
Author(s):  
A. Jorissen

An AGB star in a binary system is likely to pollute its companion with carbon- and s-process-rich matter. After the AGB star has faded into an unconspicuous white dwarf, the polluted companion enters the zoo of stars with chemical peculiarities. In this paper, the progeny of AGB stars in binary systems are identified among existing spectroscopic classes (Abell 35-like, binary post-AGB, WIRRing, dwarf Ba and C, subgiant CH, Ba, CH, S, yellow symbiotics) and their filiation is discussed from the properties of their eccentricity – period diagrams.



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