dc.creatorBenvenuto, Omar Gustavo
dc.date1987
dc.date2022-06-27T12:52:12Z
dc.date.accessioned2023-07-15T07:17:07Z
dc.date.available2023-07-15T07:17:07Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/138369
dc.identifierissn:1669-9521
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7479908
dc.descriptionWe have computed the first results of the evolution of massive stars including mass loss and overshooting (extended convection). The computation was done with a code written by us. We modified the equations of stellar structure to include both. We also present the main consequences, on the stellar structure, on the observational effects in HR diagram and in the chemical composition of the objects.
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.languagees
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectAstronomía
dc.subjectGalaxias
dc.titleEvolution of massive stars with mass loss and overshooting
dc.typeArticulo
dc.typeComunicacion


Este ítem pertenece a la siguiente institución