The galactic centre

I would like to start by bringing the good wishes of Australian radio astronomers to this new group which is joining us in the radio study of the southern sky. The nuclear regions of galaxies are generally considered as regions of high density, with population II stars in a "nuclear bulge"...

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Detalles Bibliográficos
Autor principal: Kerr, F.J.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1968
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/93068
Aporte de:
id I19-R120-10915-93068
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
Kerr, F.J.
The galactic centre
topic_facet Astronomía
Galaxias
description I would like to start by bringing the good wishes of Australian radio astronomers to this new group which is joining us in the radio study of the southern sky. The nuclear regions of galaxies are generally considered as regions of high density, with population II stars in a "nuclear bulge". In some galaxies, the presence of gas in the nucleus is shown by the appearance of the OII 3727 doublet, sometimes with a high velocity dispersion. Some nearby galaxies (e.g. M31, M33, M51) show a small very bright spot, right at the nucleus, of the order of 10 pc in diameter. Non-circular velocities have been found near the centre in some galaxies.
format Articulo
Comunicacion
author Kerr, F.J.
author_facet Kerr, F.J.
author_sort Kerr, F.J.
title The galactic centre
title_short The galactic centre
title_full The galactic centre
title_fullStr The galactic centre
title_full_unstemmed The galactic centre
title_sort galactic centre
publishDate 1968
url http://sedici.unlp.edu.ar/handle/10915/93068
work_keys_str_mv AT kerrfj thegalacticcentre
AT kerrfj galacticcentre
bdutipo_str Repositorios
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