Un estudio sobre la irregular magallánica NGC 7764
From the photographic photometry of NGC 7764, the integrated apparent magnitude and the morphological parameter qₙ was determined. From the emission lines of the spectrum the radial velocity was estimated in 1729 km/sec. The observed emission spectrum is a typical example of galaxies which show brig...
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1971
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/98022 |
| Aporte de: |
| Sumario: | From the photographic photometry of NGC 7764, the integrated apparent magnitude and the morphological parameter qₙ was determined. From the emission lines of the spectrum the radial velocity was estimated in 1729 km/sec. The observed emission spectrum is a typical example of galaxies which show brigth emission regions. |
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