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Super asymptotic giant branch stars. I - Evolution code comparison

Autor
Doherty, C.; Siess, L.; Lattanzio, J. C.; Gil Pons, P.
Tipus d'activitat
Article en revista
Revista
Monthly notices of the Royal Astronomical Society
Data de publicació
2010-01-01
Volum
401
Pàgina inicial
1453
Pàgina final
1464
Repositori
http://hdl.handle.net/2117/9195 Obrir en finestra nova
Resum
We present an extensive set of detailed stellar models in the mass range 7.7–10.5M over the metallicity range Z = 10−5–0.02. These models were produced using the Monash University version of the Mount Stromlo Stellar Structure Program (MONSTAR) and follow the evolution from the pre-main sequence to the first thermal pulse of these super asymptotic giant branch stars. A quantitative comparison is made to the study of Siess. Prior to this study, only qualitative comparisons and code validat...
Citació
Doherty, C. [et al.]. Super asymptotic giant branch stars. I - Evolution code comparison. "Monthly notices of the Royal Astronomical Society", 01 Gener 2010, vol. 401, p. 1453-1464.
Grup de recerca
DF - Dinàmica de Fluids: formació d'estructures i aplicacions geofísiques

Participants

  • Doherty, Carolyn L.  (autor)
  • Siess, Lionel  (autor)
  • Lattanzio, John C.  (autor)
  • Gil Pons, Pilar  (autor)