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dc.date.accessioned 2022-10-31T12:42:38Z
dc.date.available 2022-10-31T12:42:38Z
dc.date.issued 1992
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/144809
dc.description.abstract This paper briefly reviews some models for galaxy formation and their confrontation with observations. The analysis include the cosmological background, the clustering of mass in galactic halos, and several dynamical and photometric properties. en
dc.language es es
dc.subject Galaxia es
dc.title Formación y dinámica de galaxias es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person García-Lambas, D. 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. 37 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)