CA Tout, DS Hall - Monthly Notices of the Royal Astronomical …, 1991 - academic.oup.com
Stars in close binary systems can suffer two kinds of mass change:(1) mass transfer between the stars, and (2) mass loss completely from the system. The former process occurs when …
W Lu, J Fuller, E Quataert… - Monthly Notices of the …, 2023 - academic.oup.com
In some semidetached binary systems, the donor star may transfer mass to the companion at a very high rate. We propose that, at sufficiently high mass-transfer rates such that the …
TAF Comerford, RG Izzard, RA Booth… - Monthly Notices of the …, 2019 - academic.oup.com
Binary stars often move through an ambient medium from which they accrete material and angular momentum, as in triple-star systems, star-forming clouds, young globular clusters …
T Nagae, K Oka, T Matsuda, H Fujiwara… - Astronomy & …, 2004 - aanda.org
Three-dimensional hydrodynamic calculations are performed in order to investigate mass transfer in a close binary system, in which one component undergoes mass loss through a …
We run a numerical experiment ejecting stellar winds in a very massive binary system measuring the properties of the resulting colliding wind structure and accreted mass onto the …
MJ Plavec - International Astronomical Union Colloquium, 1981 - cambridge.org
Mass 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 …
B Jahanara, M Mitsumoto, K Oka, T Matsuda… - Astronomy & …, 2005 - aanda.org
We present three-dimensional hydrodynamic calculations of mass transfer in an interacting binary system in which one component undergoes mass loss through a wind, and does so …
SH Negu, SB Tessema - International Journal of Astronomy and …, 2015 - scirp.org
The evolution of a binary star system by various analytical and numerical approximations of mass transfer rate normalized to the equilibrium rate and its stability conditions are …
S Shiber, R Schreier, N Soker - Research in Astronomy and …, 2016 - iopscience.iop.org
Energetic outflows from main sequence stars accreting mass at very high rates might account for the powering of some eruptive objects, such as merging main sequence stars …