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Clues to type ia supernovae progenitors from degenerate carbon ignition models

Autor
Bravo, E.; Tornambé, A.; Dominguez Aguilera, Maria Inmaculada; Isern, J.
Tipus d'activitat
Article en revista
Revista
Astronomy and astrophysics
Data de publicació
1996-04
Volum
306
Número
1
Pàgina inicial
811
Pàgina final
822
Repositori
http://hdl.handle.net/2117/18904 Obrir en finestra nova
URL
http://www.aanda.org/ Obrir en finestra nova
Resum
A partially cooled 0.8 Msun_ C-O dwarf has been made accrete C + O at several accretion rates. The computed models cover the full range of possible thermal behaviours found in accreting white dwarfs. Among the models lying in the range of accretion rates for which it occurs a central carbon ignition, one has been followed in detail also along the phase between central carbon ignition and the moment in which hydrostatic equilibrium is broken. The following dynamical evolution has been computed wi...
Citació
Bravo, E. [et al.]. Clues to type ia supernovae progenitors from degenerate carbon ignition models. "Astronomy and astrophysics", Abril 1996, vol. 306, núm. 1, p. 811-822.
Paraules clau
Supernovae: General, Binaries: Close, White Dwarfs, Nuclear Reactions, Nucleosynthesis, Abundances
Grup de recerca
GRPFM - Grup de Recerca en Propietats Físiques dels Materials

Participants

  • Bravo Guil, Eduardo  (autor)
  • Tornambé, A  (autor)
  • Dominguez Aguilera, Maria Inmaculada  (autor)
  • Isern Vilaboy, Jordi  (autor)

Arxius