A new observational tracer for high-density disc-like structures around B[e] supergiants
The disc formation mechanism of B[e] supergiants is one of the puzzling phenomena in massive star evolution. Rapid stellar rotation seems to play an important role for the non-spherically symmetric mass-loss leading to a high-density disc- or ring-like structure of neutral material around these mass...
Guardado en:
Autores principales: | Aret, A., Kraus, M., Muratore, María Florencia, Borges Fernandes, M. |
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Formato: | Articulo |
Lenguaje: | Inglés |
Publicado: |
2012
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Materias: | |
Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84658 |
Aporte de: |
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