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dc.date.accessioned 2023-07-06T10:32:28Z
dc.date.available 2023-07-06T10:32:28Z
dc.date.issued 1994
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/155113
dc.description.abstract A model based on the kinetic theory is proposed for tenuous gaseous envelopes subject to a central attraction field. Quasi-steady states are studied where the gaseous system shows differential rotation. The density of particles, mean velocity of the gas and kinetic temperature are analytically determined. The kinematic behavior of the gas is analyzed in detail by studying the hydrodynamic limit of rotationally forced ejection of matter and condition of escape. en
dc.language es es
dc.subject Galaxia es
dc.title Kinetic model for diluted gaseous envelopes in a central field en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Rohrmann, René 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. 39 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)