Zobrazeno 1 - 10
of 139
pro vyhledávání: '"Donder E"'
Autor:
Katsiyannis, A. C., Dominique, M., Pierrard, V., Rosson, G. Lopez, De Keyser, J., Berghmans, D., Kruglanski, M., Dammasch, I. E., De Donder, E.
Publikováno v:
J. Space Weather Space Clim. 2018, 8, A01
Aims. To better understand the radiation environment in low Earth orbit (LEO), the analysis of in-situ observations of a variety of particles, at different atmospheric heights, and in a wide range of energies, is needed. Methods. We present an analys
Externí odkaz:
http://arxiv.org/abs/1710.04653
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
Autor:
Neefs, E., Vandaele, A.C., De Cock, R., Erwin, J., Robert, S., Thomas, I.R., Berkenbosch, S., Jacobs, L., Bogaert, P., Beeckman, B., Brassine, A., Messios, N., De Donder, E., Bolsée, D., Pereira, N., Tackley, P., Gerya, T., Kögl, S., Kögl, P., Gröbelbauer, H.-P., Wirz, F., Székely, G., Eaton, N., Roibás-Millán, E., Torralbo, I., Rubio-Arnaldo, H., Alvarez, J.M., Navajas Ortega, D., De Vos, L., Sørensen, R., Moelans, W., Algoedt, A., Blau, M., Stam, D., Renotte, E., Klinkenberg, P., Borguet, B., Thomas, S., Vervaeke, M., Thienpont, H., Castro, J.M., Jimenez, J.
Publikováno v:
In Acta Astronautica January 2025 226 Part 1:178-201
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 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
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Vanbeveren, D., De Donder, E.
Publikováno v:
New Astron. 12 (2006) 95-103
Low metallicity very massive stars with an initial mass between 140 Mo and 260 Mo can be subdivided into two groups: those between 140 Mo and 200 Mo which produce a relatively small amount of Fe, and those with a mass between 200 Mo and 260 Mo where
Externí odkaz:
http://arxiv.org/abs/astro-ph/0608337
Autor:
Vanbeveren, D., De Donder, E.
A comparison between the observed O-type star and the WR star populations and the theoretically predicted ones depends on the effects of stellar wind mass loss during various phases and rotation on stellar evolution and, last not least, on the effect
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309104
Autor:
De Donder, E., Vanbeveren, D.
Publikováno v:
New Astron. 8 (2003) 817-836
Supernova rates (hypernova, type II, type Ib/c and type Ia) in a particular galaxy depend on the metallicity (i.e. on the galaxy age), on the physics of star formation and on the binary population. In order to study the time evolution of the galactic
Externí odkaz:
http://arxiv.org/abs/astro-ph/0305462
Autor:
De Donder, E., Vanbeveren, D.
A population number synthesis code follows in detail the evolution of a population of single stars and of close binaries. We use our code to simulate the population of neutron star - neutron star and black hole - neutron star binaries. We then combin
Externí odkaz:
http://arxiv.org/abs/astro-ph/0302048