Fotometría superficial de galaxias a dos colores
For a given number of galaxies the behaviour of the form parameter qₙ in the photometric systems P and V it is described. It is found, in general, that: qₙ(V) < qₙ(P), what implies n(V ) > n (P) , i.e., the brightness distribution law in the visual (V) is associated with an earlier qₙ (consequ...
Guardado en:
| Autor principal: | |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1971
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/98072 |
| Aporte de: |
| Sumario: | For a given number of galaxies the behaviour of the form parameter qₙ in the photometric systems P and V it is described. It is found, in general, that: qₙ(V) < qₙ(P), what implies n(V ) > n (P) , i.e., the brightness distribution law in the visual (V) is associated with an earlier qₙ (consequently with an n) than the one in the photographic range. |
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