Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2022-12-14T12:46:57Z
dc.date.available 2022-12-14T12:46:57Z
dc.date.issued 1993
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/147219
dc.description.abstract We describe a code to determine the initial and present mass of a star in the HR diagram. The code is based on an interpolation procedure between the two adjacent evolutionary tracks where the star is situated according to its luminosity and temperature (from Mv and CI). With a few modifications the code may be used with any set of evolutionary tracks. The mass obtained from the present position of the star in the HR diagram, may be rather ambiguous considering that it can be positioned in any of all the possible loops predicted by the theory of the evolution. Our code takes into account all possible solutions. en
dc.language es es
dc.subject Galaxia es
dc.title A code to compute stellar masses in the HR diagram en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Baume, Gustavo Luis es
sedici.creator.person Paoli, Sergio Alejandro es
sedici.creator.person Vázquez, Rubén Ángel es
sedici.creator.person Feinstein, Alejandro es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 38 es


Descargar archivos

Thumbnail
Resumen (1 p.)
Descargar archivo (156.8Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)