PLANETARY NEBULAE II ELECTRON TEMPERATURES AND ELECTRON DENSITIES

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dc.contributor.authorPEIMBERT, M
dc.date.accessioned2026-05-28T16:31:15Z
dc.date.issued1971
dc.description.abstractThe electron temperature is obtained for thirteen planetary nebulae by means of forbidden lines of oxygen doubly ionized and nitrogen singly ionized. These temperatures range from 9000 to 15300°K. From the ratio of the Balmer continuum to the Balmer emiss
dc.description.paginacion29 - 37
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent8
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/23148
dc.language.isoInglés
dc.numero.secuencia23145
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 6
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectPLANETARY, NEBULAE, ELECTRON TEMPERATURES, ELECTRON DENSITIES
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaPLANETOLOGIA
dc.subject.subdisciplinaGEOLOGIA PLANETARIA
dc.titlePLANETARY NEBULAE II ELECTRON TEMPERATURES AND ELECTRON DENSITIES
dc.title.alternativeBOL OBS TONAN TACUB

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