Survey of helium weak stars
The spectra of a dozen stars were obtained in which the colors are bluer than expected according to their spectral types. Eight of them are helium weak. With these objects the percentage of stars of this type is increased by 50 %. The paper in full will be published elsewhere.
Guardado en:
| Autores principales: | , , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1970
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/97666 |
| Aporte de: |
| Sumario: | The spectra of a dozen stars were obtained in which the colors are bluer than expected according to their spectral types. Eight of them are helium weak. With these objects the percentage of stars of this type is increased by 50 %. The paper in full will be published elsewhere. |
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