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dc.date.accessioned 2020-08-13T12:52:03Z
dc.date.available 2020-08-13T12:52:03Z
dc.date.issued 1981
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/102202
dc.description.abstract Se analizan las curvas de luz U, B y V del sistema W UMa MW Pavonis, hallándose los elementos orbitales. El modelo de Russell permite obtener soluciones satisfactorias de las tres curvas de luz. es
dc.language es es
dc.subject Galaxias es
dc.title Análisis del sistema MW Pav es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Lapasset, E. 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. 21 es


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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)