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dc.date.accessioned 2020-05-13T14:29:54Z
dc.date.available 2020-05-13T14:29:54Z
dc.date.issued 1969
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/95816
dc.description.abstract γ₂ Velorum, the brightest Wolf-Rayet star in the sky, is a WC object with no N in its spectrum. As it has been already announced the spectrum is a double-lined one and can be described as a WC 7 + 09. The 09 star displays absorption lines of He and H, the Balmer series being visible up to H 17. The spectroscopic period has been set by Bappu as of 78.5 days, and the results of the measurement of about 1/4 of the material at our disposal -some 200 spectra taken at the Cordoba Observatory with a dispersion of 40 Å/mm and covering the region λλ 3100-6800- seem to agree with such a period. en
dc.language es es
dc.subject Galaxias es
dc.title The spectrum of γ₂ Velorum en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person de Monteagudo, V.N. 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. 14 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)