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dc.date.accessioned 2022-10-12T14:43:55Z
dc.date.available 2022-10-12T14:43:55Z
dc.date.issued 1992
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/143656
dc.description.abstract Employing the statistical analysis of Muzyliev (1978, Nauch. Inform. Astronom. Council USSR Acad. Sci. 41, 94) we have made a code for obtaining the mass of a star, if the two evolutionary tracks along which it lies are known. The code has been adapted to use it with evolutionary tracks (either with mass loss or without it). We likewise treat the ambiguous position of some stars (normally massive ones) onto the CM diagram (where the star could be describing one of the "loops" predicted by the theory). en
dc.language es es
dc.subject Galaxia es
dc.title Code for calculating the mass of a star onto the HR diagram en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Paoli, Sergio Alejandro es
sedici.creator.person Baume, Gustavo Luis 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. 37 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)


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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)