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...

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Detalles Bibliográficos
Autores principales: Pastoriza, Miriani Griselda, Agüero, Estela Laura
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1971
Materias:
Astronomía
Galaxias
NGC 7764
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/98022
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-98022
record_format dspace
spelling I19-R120-10915-980222024-04-30T17:40:17Z http://sedici.unlp.edu.ar/handle/10915/98022 Un estudio sobre la irregular magallánica NGC 7764 Pastoriza, Miriani Griselda Agüero, Estela Laura 1971 2020-06-11T12:33:57Z es Astronomía Galaxias 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 brigth emission regions. 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 7764
spellingShingle Astronomía
Galaxias
NGC 7764
Pastoriza, Miriani Griselda
Agüero, Estela Laura
Un estudio sobre la irregular magallánica NGC 7764
topic_facet Astronomía
Galaxias
NGC 7764
description 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.
format Articulo
Comunicacion
author Pastoriza, Miriani Griselda
Agüero, Estela Laura
author_facet Pastoriza, Miriani Griselda
Agüero, Estela Laura
author_sort Pastoriza, Miriani Griselda
title Un estudio sobre la irregular magallánica NGC 7764
title_short Un estudio sobre la irregular magallánica NGC 7764
title_full Un estudio sobre la irregular magallánica NGC 7764
title_fullStr Un estudio sobre la irregular magallánica NGC 7764
title_full_unstemmed Un estudio sobre la irregular magallánica NGC 7764
title_sort un estudio sobre la irregular magallánica ngc 7764
publishDate 1971
url http://sedici.unlp.edu.ar/handle/10915/98022
work_keys_str_mv AT pastorizamirianigriselda unestudiosobrelairregularmagallanicangc7764
AT agueroestelalaura unestudiosobrelairregularmagallanicangc7764
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