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dc.date.accessioned 2020-04-08T11:59:52Z
dc.date.available 2020-04-08T11:59:52Z
dc.date.issued 1968
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/93068
dc.description.abstract 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. en
dc.language es es
dc.subject Galaxias es
dc.title The galactic centre en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Kerr, F.J. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no.11 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)