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: | , , , , , , , |
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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: |
Sumario: | 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. |
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