The spectroscopic orbits and physical parameters of GG car
GG Car is a peculiar B type star with emission lines classified as a B[e] supergiant star. In this work we present a spectral analysis of this system based on spectra obtained at Casleo. We fit the spectral energy distribution adopting a model for the gas and dust circumstellar components and thus w...
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| Autores principales: | Marchiano, Paula Esther, Brandi, Estela, Muratore, María Florencia, Quiroga, Claudio Hugo Martín, Ferrer, Osvaldo Eduardo, García, Lía Guillermina |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Inglés |
| Publicado: |
2011
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/85612 |
| Aporte de: |
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