THE SAN LUIS POTOSIECTRUM OF R CORONAE AUSTRALIS

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dc.contributor.authorMENDOZA, EUGENIO
dc.contributor.authorJASCHEK, M
dc.contributor.authorJASCHEK, C
dc.date.accessioned2026-05-28T16:30:13Z
dc.date.issued1970
dc.description.abstractThe spectrum of R CrA cannot be classified uniquely in the MK system. However, the K-line of Ca II and some hydrogen lines indicate a spectral type earlier than A7, perhaps A5. Shell characteristics, with extremely strong Ti II (specially ??3759-61) are o
dc.description.paginacion107 - 109
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent3
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22745
dc.language.isoInglés
dc.numero.secuencia22742
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 5
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectSPECTRUM, CORONAE AUSTRALIS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleTHE SAN LUIS POTOSIECTRUM OF R CORONAE AUSTRALIS
dc.title.alternativeBOL OBS TONAN TACUB

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