THE SELFABSORPTION SAN LUIS POTOSIECTRUM OF THE TRIPLET SYSTEM OF HE I

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dc.contributor.authorBLOCK, RA
dc.date.accessioned2026-05-28T15:58:09Z
dc.date.issued1968
dc.description.abstractThe relative line intensities for the triplet system in He I, have been re-computed for various nebular optical depths at ?3888. The profile of the line has been considered due to its importance. The electron collisions have not been taken into account si
dc.description.paginacion210 - 214
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent5
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/21958
dc.language.isoInglés
dc.numero.secuencia21955
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectSELF, ABSORPTION SPECTRUM, TRIPLET SYSTEM
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleTHE SELFABSORPTION SAN LUIS POTOSIECTRUM OF THE TRIPLET SYSTEM OF HE I
dc.title.alternativeBOL OBS TONAN TACUB

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