A new hot subdwarf
HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this group and also the only one known spectroscopic binary. The complete paper will appear in the "Publications of the Astronomical Society of the Pacific".
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Inglés |
| Publicado: |
1963
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/91599 |
| Aporte de: |
| Sumario: | HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this group and also the only one known spectroscopic binary. The complete paper will appear in the "Publications of the Astronomical Society of the Pacific". |
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