The HII regions in galaxies
The correlation between morphological type and the diameters of the largest HII complexes in galaxies is interpreted theoretically as a consequence of the rate of stellar formation of massive stars and the original luminosity function in galaxies.
Guardado en:
| Autor principal: | |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Inglés |
| Publicado: |
1963
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/91651 |
| Aporte de: |
| Sumario: | The correlation between morphological type and the diameters of the largest HII complexes in galaxies is interpreted theoretically as a consequence of the rate of stellar formation of massive stars and the original luminosity function in galaxies. |
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