The impact of radiation and wind momenta on mass transfer in massive close binary systems

L Dessart, N Langer, J Petrovic - Astronomy & Astrophysics, 2003 - aanda.org
We investigate to what extent the radiation and stellar wind momenta in a massive close
binary system can remove part of the matter flowing from one towards the other star during a …

Wind driven mass transfer in interacting binary systems

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 …

On rapid binary mass transfer–I. Physical model

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 …

Bondi–Hoyle–Lyttleton accretion by binary stars

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 …

Wind accretion in binary stars-I. Mass accretion ratio

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 …

[HTML][HTML] Numerical Study of Colliding Winds in Massive Stars

A Kashi, A Michaelis - Galaxies, 2021 - mdpi.com
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 …

Mass loss from interacting close binary systems

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 …

Wind accretion in binary stars-II. Angular momentum loss

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 …

[HTML][HTML] Mass transfer in binary stellar evolution and its stability

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 …

Binary interactions with high accretion rates onto main sequence stars

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 …