The influence of mass-transfer variability on the growth of white dwarfs, and the implications for Type Ia supernova rates
- Toonen, S.
- Voss, R.
- Knigge, C.
DOIAbstract
Contains fulltext : 127905.pdf (preprint version ) (Open Access
Contains fulltext : 127905.pdf (preprint version ) (Open Access
Contains fulltext : 156239.pdf (preprint version ) (Open Access
The theoretical and observed populations of pre-cataclysmic variables are dominated by systems with ...
Context. Mass transfer stability is a key issue in studies of binary evolution. Critical mass ratios...
White dwarfs (WDs) can increase their mass by accretion from companion stars, provided the mass-accr...
Contains fulltext : 91460.pdf (preprint version ) (Open Access
Type Ia supernovae, sparked off by exploding white dwarfs of mass close to the Chandrasekhar limit, ...
Contains fulltext : 156097.pdf (preprint version ) (Open Access
“Copyright 2011 American Institute of Physics. This article may be downloaded for personal use only....
Contains fulltext : 103792.pdf (preprint version ) (Open Access
Abstract. Recent observations of high-z SNe Ia provide evidence that the Universe is accelerating du...
Context. The study of Type Ia supernovae (SNIa) has lead to greatly improved insights into...
10 pages, 2 tables.-- En: "Supernovae: lights in the darkness", October 3-5, 2007, Mao (Menorca), t...
Aims. Gravitational settling of 22Ne in cooling white dwarfs can affect the outcome of thermonuclear...
The following full text is a preprint version which may differ from the publisher's version
We investigate variations of the mass transfer rate in cataclysmic variables (CVs) that are induced ...
Contains fulltext : 156239.pdf (preprint version ) (Open Access
The theoretical and observed populations of pre-cataclysmic variables are dominated by systems with ...
Context. Mass transfer stability is a key issue in studies of binary evolution. Critical mass ratios...
White dwarfs (WDs) can increase their mass by accretion from companion stars, provided the mass-accr...
Contains fulltext : 91460.pdf (preprint version ) (Open Access
Type Ia supernovae, sparked off by exploding white dwarfs of mass close to the Chandrasekhar limit, ...
Contains fulltext : 156097.pdf (preprint version ) (Open Access
“Copyright 2011 American Institute of Physics. This article may be downloaded for personal use only....
Contains fulltext : 103792.pdf (preprint version ) (Open Access
Abstract. Recent observations of high-z SNe Ia provide evidence that the Universe is accelerating du...
Context. The study of Type Ia supernovae (SNIa) has lead to greatly improved insights into...
10 pages, 2 tables.-- En: "Supernovae: lights in the darkness", October 3-5, 2007, Mao (Menorca), t...
Aims. Gravitational settling of 22Ne in cooling white dwarfs can affect the outcome of thermonuclear...
The following full text is a preprint version which may differ from the publisher's version
We investigate variations of the mass transfer rate in cataclysmic variables (CVs) that are induced ...
Contains fulltext : 156239.pdf (preprint version ) (Open Access
The theoretical and observed populations of pre-cataclysmic variables are dominated by systems with ...
Context. Mass transfer stability is a key issue in studies of binary evolution. Critical mass ratios...
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