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dc.date.accessioned 2022-06-14T12:03:52Z
dc.date.available 2022-06-14T12:03:52Z
dc.date.issued 1987
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/137801
dc.description.abstract Low-dispersion spectra of V CrA and Y Mus are described with some detail. They correspond to hydrogen deficient carbon stars, according to their membership to the R CrB-type variable group. These spectra are classified in the C-system of Keenan and Morgan (1941), following the procedure of Yamashita(1967). It was found that V CrA and Y Mus are C1,2 and C1,0 respectively. The temperatures derived are in agreement with other determinations. en
dc.language es es
dc.subject Galaxias es
dc.subject v cra es
dc.subject y mus es
dc.title Spectral classification of V CrA and Y Mus en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Minniti, D. 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) 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)