The evolution of low-mass close binary systems. IV - 0.80 solar mass + 0.40 solar mass - Catastrophic mass loss

1977 ◽  
Vol 211 ◽  
pp. 881 ◽  
Author(s):  
R. F. Webbink
1989 ◽  
Vol 107 ◽  
pp. 361-361
Author(s):  
M.J. Sarna ◽  
A.V. Fedorova

AbstractWe investigated the effect of mass accretion on the secondary components in close binomy systems (Mtotal ≤ 2.5M⊙M2.0 ≤ 0.75M⊙) exchanging mass in the case A.


1988 ◽  
Vol 328 ◽  
pp. 617 ◽  
Author(s):  
P. N. McDermott ◽  
Ronald E. Taam ◽  
F. A. Ringwald

1981 ◽  
Vol 59 ◽  
pp. 431-456
Author(s):  
Mirek J. Plavec

AbstractMass outflow from interacting close binary systems, accompanied by loss of orbital angular momentum, appears to be a very important process affecting the evolution of binary stars. Together with accretion on the mass-gaining component, it is the least understood aspect of the general complex process we call “evolution with mass transfer and/or mass loss”, or, more briefly, “interaction”. It is therefore very imperative to assemble and examine all available facts or hints about mass loss.


2005 ◽  
Vol 326 (10) ◽  
pp. 944-947 ◽  
Author(s):  
R. D. Jeffries ◽  
P. F. L. Maxted

Sign in / Sign up

Export Citation Format

Share Document