Determination of rotational velocities in B and Be stars: physical processes and methods
In the present work we have used the method suggested by Carrol (1933) for the determination of the projected equatorial rotation velocity: v sin(i) by means of the Fourier Transform of a sample of B8 to B9.5 spectral type stars and luminosity classes III and V with Be and Bn type stars among them,...
Guardado en:
| Autores principales: | Díaz, A, Ringuelet, Adela Emilia |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1990
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/143243 |
| Aporte de: |
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