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dc.date.accessioned 2020-06-09T14:38:25Z
dc.date.available 2020-06-09T14:38:25Z
dc.date.issued 1970
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/97840
dc.description.abstract It has been studied the formation of the continuum of nebular hydrogen when ionization is due to radiation and to collisions. Two photon emission and continuous emissivity in the reaction of formation of H- have been included. The continuum results extremely sensitive to the relative amount of the two types of thermal excitation. en
dc.language es es
dc.subject Galaxias es
dc.title Theory of the continuous spectrum of gaseous nebula of pure hydrogen en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Gerola, H. 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. 15 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)