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dc.date.accessioned | 2020-06-26T14:15:22Z | |
dc.date.available | 2020-06-26T14:15:22Z | |
dc.date.issued | 1980 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/99238 | |
dc.description.abstract | It is found that is unnecessary to deal with circumstellar shells to explain the apparent correlation between reddening and luminosity in young stellar groups. The simple combination of the luminosity function and a color excess distribution can reproduce the observed appearance of the luminosity vs. color excess diagram of Cygnus II including the lack of little reddened high luminosity stars. | en |
dc.language | es | es |
dc.subject | Galaxias | es |
dc.title | Sobre la correlación entre exceso de color y luminosidad | es |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Marraco, Hugo Gustavo | 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. 18 | es |