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dc.date.accessioned 2020-03-25T11:05:31Z
dc.date.available 2020-03-25T11:05:31Z
dc.date.issued 1963
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/91599
dc.description.abstract HD 49798 was found to be a hot subdwarf. It is, at the present time the brightest member of this group and also the only one known spectroscopic binary. The complete paper will appear in the "Publications of the Astronomical Society of the Pacific". en
dc.format.extent 32-32 es
dc.language en es
dc.subject estrella subenana es
dc.title A new hot subdwarf en
dc.type Articulo es
sedici.creator.person Jaschek, Mercedes es
sedici.creator.person Jaschek, Carlos es
sedici.subject.materias Ciencias Astronómicas 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.event VI Reunión Científica de la Asociación Argentina de Astronomía (Horco Molle, Tucumán, 22 al 25 de mayo de 1963) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 6 es
dc.rights.uri http://creativecommons.org/licenses/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)