Análisis espectroscópico de la estrella peculiar tipo O,HD 49798
On the basis of material taken at Bosque Alegre, (dispresion 42 A/nm), this star shows the following peculiarities: a) the approximate spectral type is O7; b) the Balmer series is visible up to n=9; c) the He I series is very weak for the spectral type; d) the Pickering series is very much enhanced...
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1963
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/90979 |
| Aporte de: |
| Sumario: | On the basis of material taken at Bosque Alegre, (dispresion 42 A/nm), this star shows the following peculiarities:
a) the approximate spectral type is O7; b) the Balmer series is visible up to n=9; c) the He I series is very weak for the spectral type; d) the Pickering series is very much enhanced; e) there are abnormalities in other elements: nitrogen is slightly enhanced, oxygen practically absent and carbon is very weak. According to the Stark effect in the Balmer series, the star appears to be sub-luminous. The paper will be published in full elsewhere. |
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