Molecular emission from GG Carinae's circumbinary disk
Context. The appearance of the B[e] phenomenon in evolved massive stars such as B[e] supergiants is still a mystery. While these stars are generally found to have disks that are cool and dense enough for efficient molecule and dust condensation, the origin of the disk material is still unclear. Aims...
Guardado en:
| Autores principales: | Kraus, M., Oksala, M. E., Nickeler, D. H., Muratore, María Florencia, Borges Fernandes, M., Aret, A., Cidale, Lydia Sonia, De Wit, W. J. |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2012
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84418 |
| Aporte de: |
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