Code for calculating the mass of a star onto the HR diagram
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...
Guardado en:
| Autores principales: | , , , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1992
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/143656 |
| Aporte de: |
| Sumario: | 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). |
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