Browsing by Subject "stars: general"
Now showing items 1-4 of 4
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Mixing in massive stellar mergers
(Oxford University Press, 2007-09-21)The early evolution of dense star clusters is possibly dominated by close interactions between stars, and physical collisions between stars may occur quite frequently. Simulating a stellar collision event can be an intensive ... -
Stability and Coalescence of Massive Twin Binaries
(The American Astronomical Society., 2015-06-12)Massive stars are usually found in binaries, and binaries with periods less than 10 days may have a preference for near equal component masses ("twins"). In this paper we investigate the evolution of massive twin binaries ... -
Twin Binaries: Studies of Stability, Mass Transfer, and Coalescence
(Institute of Physics, 2011-08-20)Motivated by suggestions that binaries with almost equal-mass components (“twins”) play an important role in the formation of double neutron stars and may be rather abundant among binaries, we study the stability of ... -
Twin Binaries: Studies of Stability, Mass Transfer, and Coalescence
(IOP, 2011-07-28)Motivated by suggestions that binaries with almost equal-mass components ("twins") play an important role in the formation of double neutron stars and may be rather abundant among binaries, we study the stability of ...