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dc.date.accessioned 2020-07-07T13:35:34Z
dc.date.available 2020-07-07T13:35:34Z
dc.date.issued 1975
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/100096
dc.description.abstract An efficient method of Identification of spectra on objective prim plates is described. 172 early-type stars of a region in Canis Major were classified in the MK system applying this method. Only 29 of them have been classified previously in this system by other authors, with good agreement in spite of different sources. A comparison with the HD spectral types in this sky region shows them to be, on the average, one spectral subclass later than the MK types assigned in this paper. %U http://sedici.unlp.edu.ar/handle/10915/76704 en
dc.language es es
dc.subject Galaxias es
dc.title Clasificacíón espectral sobre placas con prisma objetivo es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Claría, 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. 19 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)