Unstable groups of galaxies

The observed relationship between mass-luminosity ratios for groups and clusters of galaxies and their population is interpreted on basis of a model developed by the author (1968) in which unstable groups of galaxies are thought to be the result of the fragmentation of a parent galaxy.

Guardado en:
Detalles Bibliográficos
Autor principal: Sérsic, J.L.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1969
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/95208
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-95208
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxias
spellingShingle Astronomía
Galaxias
Sérsic, J.L.
Unstable groups of galaxies
topic_facet Astronomía
Galaxias
description The observed relationship between mass-luminosity ratios for groups and clusters of galaxies and their population is interpreted on basis of a model developed by the author (1968) in which unstable groups of galaxies are thought to be the result of the fragmentation of a parent galaxy.
format Articulo
Comunicacion
author Sérsic, J.L.
author_facet Sérsic, J.L.
author_sort Sérsic, J.L.
title Unstable groups of galaxies
title_short Unstable groups of galaxies
title_full Unstable groups of galaxies
title_fullStr Unstable groups of galaxies
title_full_unstemmed Unstable groups of galaxies
title_sort unstable groups of galaxies
publishDate 1969
url http://sedici.unlp.edu.ar/handle/10915/95208
work_keys_str_mv AT sersicjl unstablegroupsofgalaxies
bdutipo_str Repositorios
_version_ 1764820491468537858

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