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pro vyhledávání: '"Greve, J. P."'
Autor:
Van Rensbergen, W., De Greve, J. P.
Publikováno v:
A&A 592, A151 (2016)
There are only a few Algols with measured accretion disk parameters. These measurements provide additional constraints for tracing the origin of individual systems, narrowing down the initial parameter space. We investigate the origin and evolution o
Externí odkaz:
http://arxiv.org/abs/1604.07589
Akademický článek
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From the eclipsing binary VW Cep, 1963 epochs of primary and secondary minima have been registered since 1926. Because VW Cep is a shallow contact binary the direction of the flow from one component to the other could possibly be reversed. We aim to
Externí odkaz:
http://arxiv.org/abs/1306.2180
Publikováno v:
MmSAI 84, 153 (2013)
The chemical processes during the Asymptotic Giant Branch (AGB) evolution of intermediate mass single stars predict most of the observations of the different populations in Globular Clusters although some important issues still need to be further cla
Externí odkaz:
http://arxiv.org/abs/1301.2423
We investigate the contribution to the formation of type Ia supernovae of the single (a white dwarf accreting from a non-degenerate companion) and double (two merging white dwarfs) degenerate scenario, as well as various aspects of the binary evoluti
Externí odkaz:
http://arxiv.org/abs/1212.0313
Publikováno v:
IAUS 281, 232 (2013)
Using a population number synthesis code with detailed binary evolution, we calculate the distribution of the number of type Ia supernovae as a function of time after starburst. This is done for both main progenitor scenarios (single degenerate and d
Externí odkaz:
http://arxiv.org/abs/1204.4358
Publikováno v:
A&A 543, A4 (2012)
Context. The chemical processes during the Asymptotic Giant Branch (AGB) evolution of intermediate mass single stars predict most of the observations of the different populations in globular clusters although some important issues still need to be fu
Externí odkaz:
http://arxiv.org/abs/1109.2713
Publikováno v:
AIPC 1314, 239 (2010)
Two formation scenarios are investigated for type Ia supernovae in elliptical galaxies: the single degenerate scenario (a white dwarf reaching the Chandrasekhar limit through accretion of matter transferred from its companion star in a binary) and th
Externí odkaz:
http://arxiv.org/abs/1009.5175
Publikováno v:
A&A 528, A16 (2011)
Liberal evolution of interacting binaries has been proposed previously by several authors in order to meet various observed binary characteristics better than conservative evolution does. Since Algols are eclipsing binaries the distribution of their
Externí odkaz:
http://arxiv.org/abs/1008.2620
Publikováno v:
A&A 515, A89 (2010)
We investigate the contribution of different formation scenarios for type Ia supernovae in elliptical galaxies. The single degenerate scenario (a white dwarf accreting from a late main sequence or red giant companion) is tested against the double deg
Externí odkaz:
http://arxiv.org/abs/1003.2491