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dc.date.accessioned | 2022-08-30T14:50:09Z | |
dc.date.available | 2022-08-30T14:50:09Z | |
dc.date.issued | 1994 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/141258 | |
dc.description.abstract | We study special aspects of the N-body problem with masses varying according to the Eddington-Jeans law with powers n=2 and 3. Our main result is that a particular set of variables can be found that allows one to write the pertinent Boltzmann and Poisson equations in a fashion similar to that corresponding to the usual fixed mass situation. | en |
dc.format.extent | 201-208 | es |
dc.language | en | es |
dc.subject | Variable mass | es |
dc.subject | Boltzmann equation | es |
dc.subject | Galaxies | es |
dc.subject | Star clusters | es |
dc.title | Boltzmann equation approach to the N-body problem with masses varying according to the Eddington-Jeans law | en |
dc.type | Articulo | es |
sedici.identifier.other | doi:10.1007/bf00692871 | es |
sedici.identifier.issn | 0923-2958 | es |
sedici.identifier.issn | 1572-9478 | es |
sedici.creator.person | Plastino, Ángel Ricardo | es |
sedici.creator.person | Muzzio, Juan Carlos | es |
sedici.subject.materias | Astronomía | es |
sedici.subject.materias | Ciencias Exactas | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Facultad de Ciencias Astronómicas y Geofísicas | es |
sedici.subtype | Articulo | es |
sedici.rights.license | Creative Commons Attribution 4.0 International (CC BY 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
sedici.description.peerReview | peer-review | es |
sedici.relation.journalTitle | Celestial Mechanics & Dynamical Astronomy | es |
sedici.relation.journalVolumeAndIssue | vol. 59, no. 3 | es |