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dc.date.accessioned 2020-03-25T13:53:47Z
dc.date.available 2020-03-25T13:53:47Z
dc.date.issued 1963
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/91651
dc.description.abstract The correlation between morphological type and the diameters of the largest HII complexes in galaxies is interpreted theoretically as a consequence of the rate of stellar formation of massive stars and the original luminosity function in galaxies. en
dc.language en es
dc.subject Galaxias es
dc.title The HII regions in galaxies en
dc.type Articulo es
sedici.creator.person Sérsic, José Luis 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)