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dc.date.accessioned 2020-04-28T11:48:46Z
dc.date.available 2020-04-28T11:48:46Z
dc.date.issued 1969
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/94437
dc.description.abstract The W UMa system of ε Coronae Austrinae only shows the spectrum of one of the components which corresponds to type FOV. Since the amplitudes of the two light minima are approximately equal, the two components must have comparable surface brightness and, as a consequence, the fact that only one spectrum shows must mean that the two stars that form the system are of very similar spectral type and of different dimensions. We may be dealing with a system the interpretation of which may be important to understand evolution in close binaries. en
dc.language es es
dc.subject Galaxias es
dc.title Órbita de ε Coronae Austrinae es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Hernández, Carlos A. es
sedici.creator.person Sahade, Jorge 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. 12 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)