Interplay between pulsations and mass loss in the blue supergiant 55 Cygnus = HD 198 478
Context. Blue supergiant stars are known to display photometric and spectroscopic variability that is suggested to be linked to stellar pulsations. Pulsational activity in massive stars strongly depends on the star's evolutionary stage and is assumed to be connected with mass-loss episodes, the...
Guardado en:
| Autores principales: | Kraus, M., Haucke, M., Cidale, Lydia Sonia, Venero, Roberto Oscar José, Nickeler, D. H., Németh, P., Niemczura, E., Tomić, S., Aret, A., Kubát, J., Kubátová, B., Oksala, M. E., Curé, M., Kamiński, K., Dimitrov, W., Fagas, M., Polińska, M. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2015
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/86396 |
| Aporte de: |
Ejemplares similares
-
Wind properties of variable B supergiants : Evidence of pulsations connected with mass-loss episodes
por: Haucke, Maximiliano, et al.
Publicado: (2018) -
The Slow Winds of A-Type Supergiants
por: Granada, Anahí, et al.
Publicado: (2010) -
Resolving the kinematics of the discs around Galactic B[e] supergiants
por: Maravelias, G., et al.
Publicado: (2018) -
Discovery of the first B[e] supergiants in M 31
por: Kraus, M., et al.
Publicado: (2014) -
Dense molecular environments of B[e] supergiants and yellow hypergiants
por: Kraus, Michaela, et al.
Publicado: (2023)