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:
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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: |
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I19-R120-10915-98072 |
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I19-R120-10915-980722024-04-30T18:34:13Z http://sedici.unlp.edu.ar/handle/10915/98072 Fotometría superficial de galaxias a dos colores Agüero, Estela Laura 1971 2020-06-11T15:40:32Z es Astronomía Galaxias NGC 4374 ngc 4406 ngc 4435 ngc 4438 ngc 4459 ngc 4474 ngc 4501 ngc 4696 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. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Español |
| topic |
Astronomía Galaxias NGC 4374 ngc 4406 ngc 4435 ngc 4438 ngc 4459 ngc 4474 ngc 4501 ngc 4696 |
| spellingShingle |
Astronomía Galaxias NGC 4374 ngc 4406 ngc 4435 ngc 4438 ngc 4459 ngc 4474 ngc 4501 ngc 4696 Agüero, Estela Laura Fotometría superficial de galaxias a dos colores |
| topic_facet |
Astronomía Galaxias NGC 4374 ngc 4406 ngc 4435 ngc 4438 ngc 4459 ngc 4474 ngc 4501 ngc 4696 |
| description |
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. |
| format |
Articulo Comunicacion |
| author |
Agüero, Estela Laura |
| author_facet |
Agüero, Estela Laura |
| author_sort |
Agüero, Estela Laura |
| title |
Fotometría superficial de galaxias a dos colores |
| title_short |
Fotometría superficial de galaxias a dos colores |
| title_full |
Fotometría superficial de galaxias a dos colores |
| title_fullStr |
Fotometría superficial de galaxias a dos colores |
| title_full_unstemmed |
Fotometría superficial de galaxias a dos colores |
| title_sort |
fotometría superficial de galaxias a dos colores |
| publishDate |
1971 |
| url |
http://sedici.unlp.edu.ar/handle/10915/98072 |
| work_keys_str_mv |
AT agueroestelalaura fotometriasuperficialdegalaxiasadoscolores |
| _version_ |
1807220559944089600 |