Intriguing detection of ¹²CO molecular emission in a classical Be star
In the group of B stars with spectroscopic peculiarities, we can find the Be and the B[e] stars. The Be stars are early-type rapid rotators that present, as their principal characteristic, emission lines of hydrogen and singly ionized metals due to the presence of a gaseous envelope. The B[e] stars...
Guardado en:
| Autores principales: | Cochetti, Yanina Roxana, Arias, María Laura, Kraus, Michaela, Cidale, Lydia Sonia, Torres, Andrea Fabiana, Granada, A., Maryeva, O. V. |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/125601 |
| Aporte de: |
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