Influencia de la dispersión atmosférica e instrumental en la distribución de brillo de una galaxia
It is demonstrated that a generalized de Vaucouleurs law of brightness distribution is conserved after a smearing of gaussian profile at least in the first approximation.
Guardado en:
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| Formato: | Articulo |
| Lenguaje: | Español |
| Publicado: |
1963
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/91601 |
| Aporte de: |
| Sumario: | It is demonstrated that a generalized de Vaucouleurs law of brightness distribution is conserved after a smearing of gaussian profile at least in the first approximation. |
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