MOLECULAR HYDROGEN AND THE ULTRAVIOLET RADIATION OF SUPERNOVAE

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dc.contributor.authorPOVEDA, ARCADIO
dc.date.accessioned2026-05-28T15:51:32Z
dc.date.issued1961
dc.description.abstractWe aim to establish a limiting value to the abundance of molecular hydrogen through the indirect evidence obtained from the phenomenon of a supernova explosion. We conclude that in the vicinity of the Crab Nebula, the molecular density is smaller than 1.5
dc.description.paginacion119 - 124
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent6
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/19746
dc.language.isoInglés
dc.numero.secuencia19743
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 3
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectMOLECULAR, HYDROGEN, ULTRAVIOLET, RADIATION, SUPERNOVAE
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaRAYOS ULTRAVIOLETA
dc.titleMOLECULAR HYDROGEN AND THE ULTRAVIOLET RADIATION OF SUPERNOVAE
dc.title.alternativeBOL OBS TONAN TACUB

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