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...

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Detalles Bibliográficos
Autores principales: Aret, A., Kraus, M., Muratore, María Florencia, Borges Fernandes, M.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2012
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/84658
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