In this thesis, I present the results of hydrodynamical modelling of wind-mass transfer during the asymptotic giant branch phase of low- and intermediate-mass binary stars, with the aim of understanding the impact on the orbital evolution of the system
We present a rapid binary-evolution algorithm that enables modelling of even the most complex binary...
We investigate to what extent the radiation and stellar wind momenta in a massive close binary syste...
Low- and intermediate mass stars move up the asymptotic giant branch (AGB) as they reach the end of ...
Carbon-enhanced metal-poor stars, CH stars, barium stars, and extrinsic S stars, among other classes...
Context. The late evolutionary phase of low- and intermediate-mass stars is strongly constrained by ...
Contains fulltext : 202997.pdf (publisher's version ) (Open Access)Radboud Univers...
Wind mass transfer in binary systems with asymptotic giant branch (AGB) donor stars plays a fundamen...
Abstract: The results of 2D gas-dynamic calculation of mass transfer in binaries with com...
This thesis work is concerned with the accretion processes and flow structures associated with stell...
Using the model by Keppens (1997), we investigate the angular momentum (AM) evolution in asymmetric ...
The connection of stellar winds to many astrophysical problems ranges from star formation, through s...
Abstract: Before binary components interact, they evolve as single stars do. We therefore first crit...
We present three-dimensional hydrodynamic calculations of mass transfer in an interacting binary sy...
Context. In binary star systems, the winds from the two components impact each other, leading to str...
Context. Massive stars with solar metallicity lose important amounts of rotational angular momentum ...
We present a rapid binary-evolution algorithm that enables modelling of even the most complex binary...
We investigate to what extent the radiation and stellar wind momenta in a massive close binary syste...
Low- and intermediate mass stars move up the asymptotic giant branch (AGB) as they reach the end of ...
Carbon-enhanced metal-poor stars, CH stars, barium stars, and extrinsic S stars, among other classes...
Context. The late evolutionary phase of low- and intermediate-mass stars is strongly constrained by ...
Contains fulltext : 202997.pdf (publisher's version ) (Open Access)Radboud Univers...
Wind mass transfer in binary systems with asymptotic giant branch (AGB) donor stars plays a fundamen...
Abstract: The results of 2D gas-dynamic calculation of mass transfer in binaries with com...
This thesis work is concerned with the accretion processes and flow structures associated with stell...
Using the model by Keppens (1997), we investigate the angular momentum (AM) evolution in asymmetric ...
The connection of stellar winds to many astrophysical problems ranges from star formation, through s...
Abstract: Before binary components interact, they evolve as single stars do. We therefore first crit...
We present three-dimensional hydrodynamic calculations of mass transfer in an interacting binary sy...
Context. In binary star systems, the winds from the two components impact each other, leading to str...
Context. Massive stars with solar metallicity lose important amounts of rotational angular momentum ...
We present a rapid binary-evolution algorithm that enables modelling of even the most complex binary...
We investigate to what extent the radiation and stellar wind momenta in a massive close binary syste...
Low- and intermediate mass stars move up the asymptotic giant branch (AGB) as they reach the end of ...
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