Modeling of emission lines in low-ionization winds of B-type stars
Motivated by the availability of new observational material provided by Gaia mission, and focused on peculiar B-type stars, we develop a model to simulate the non-LTE line profiles of ionized elements such as Ca π and Mg II. The calculation is performed for a range of effective temperature and surfa...
Guardado en:
| Autores principales: | Mercanti, Lorena Verónica, Cidale, Lydia Sonia, Torres, Andrea Fabiana, Cochetti, Yanina Roxana, Kraus, M. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/166629 |
| Aporte de: |
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