Discovery of Raman-scattered lines in the massive luminous emission-line: Star LHA 115-S 18
LHA 115-S 18 is a very peculiar emission-line star exhibiting the B[e] phenomenon. Located in the Small Magellanic Cloud, its spectrum shows features of an extremely wide range of excitation and ionization stages, extending from highly ionized atomic lines (Si IV, CIV, HeII) in the ultraviolet and o...
Guardado en:
| Autores principales: | Torres, Andrea Fabiana, Kraus, M., Cidale, Lydia Sonia, Barbá, Rodolfo Héctor, Borges Fernandes, M., Brandi, Estela |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2012
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84551 |
| Aporte de: |
Ejemplares similares
-
Resolving the clumpy circumstellar environment of the B[e] supergiant LHA 120-S 35
por: Torres, Andrea Fabiana, et al.
Publicado: (2018) -
The sudden appearance of CO emission in LHA 115-S 65
por: Oksala, M. E., et al.
Publicado: (2012) -
Inhomogeneous molecular ring around the B[e] supergiant LHA 120-S 73
por: Kraus, M., et al.
Publicado: (2016) -
Discovery of SiO band emission from galactic B[e] supergiants
por: Kraus, M., et al.
Publicado: (2015) -
Discovery of the first B[e] supergiants in M 31
por: Kraus, M., et al.
Publicado: (2014)