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dc.date.accessioned 2022-11-01T14:06:33Z
dc.date.available 2022-11-01T14:06:33Z
dc.date.issued 1992
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/144898
dc.description.abstract Aguilar and Merritt (1990, Ap. J., 354, 33) have showed that the radial orbit instability, by building up triaxial systems, plays a crucial role in the galaxy formation by dissipationless colapse. We show here that Hubble's expansion and the inhomogeneity of the material may be an alternative way of preventing bar formation, instead of velocity dispersion or rotation of the material. en
dc.language es es
dc.subject Galaxia es
dc.title La inestabilidad de órbitas radiales en la formación de galaxias por colapso no disipativo es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Carpintero, Daniel Diego es
sedici.creator.person Muzzio, Juan Carlos es
sedici.creator.person Wachlin, Felipe Carlos 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)