Spectroscopic and interferometric approach for differential rotation in massive fast rotators
The coupling between the convective region in the envelope and rotation can produce a surface latitudinal differential rotation that may induce changes of the stellar geometry and on the spectral line profiles that it may be scrutinized spectroscopically and by interferometry.
Guardado en:
| Autores principales: | Zorec, Juan, Frémat, Yves, Delaa, Omar, De Souza, Armando Domiciano, Stee, Philippe, Mourard, Denis, Cidale, Lydia Sonia, Martayan, Christophe |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Inglés |
| Publicado: |
2011
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84073 |
| Aporte de: |
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