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dc.date.accessioned 2022-08-30T12:53:06Z
dc.date.available 2022-08-30T12:53:06Z
dc.date.issued 1987
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/141221
dc.description.abstract The UBV photometry of the short period binary FM Vel is analysed by means of the method of Wilson and Devinney. As the spectral type (F8) of the system represents the limit between the A and W sub-classes of contact binaries, both configurations are investigated. The results show that FM Vel has the typical features of the W type of W UMa system. The photometric value of the mass ratio is estimated around 2.0±0.2 and a degree of over-contact of about 16% is found. Both components are thermally coupled. en
dc.language es es
dc.subject Galaxia es
dc.subject fm vel es
dc.title FM Velorum: a W Ursae majoris system of W-type en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Gómez, M. es
sedici.creator.person Lapasset, E. es
sedici.creator.person Clariá, J.J. 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. 33 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) 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)