Near-infrared Characterization of Four Massive Stars in Transition Phases
Massive stars typically undergo short-lived post-main sequence evolutionary phases with strong mass loss and occasional mass eruptions. Many of such massive stars in transition phases have been identified based on their dusty envelopes. The ejected material often veils the stellar photospheres so th...
Guardado en:
| Autores principales: | Cochetti, Yanina Roxana, Kraus, Michaela, Arias, María Laura, Cidale, Lydia Sonia, Eenmäe, Tõnis, Liimets, T., Torres, Andrea Fabiana, Djupvik, A. A. |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2020
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/128616 |
| Aporte de: |
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