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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 |