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dc.date.accessioned 2020-06-11T12:48:03Z
dc.date.available 2020-06-11T12:48:03Z
dc.date.issued 1971
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/98026
dc.description.abstract The relative intensities of the hydrogen emission lines of homogeneous gaseous nebulae, ionized and excited by riative and collisional processes, have been calculated. The results define allowed and forbidden regions in the Balmer colour-colour plot different from those obtained assuming purely radiative or purely collisional excitation and ionization. A brief comparison with observational data is carried out. en
dc.language es es
dc.subject Galaxias es
dc.title The hydrogen line spectrum of gaseous nebulae en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Gerola, H. es
sedici.creator.person Salem, M. es
sedici.creator.person Panagia, N. 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. 16 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)