NOTE ON THE WY VELORUM SAN LUIS POTOSIECTRUM

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dc.contributor.authorMUNCH, LUIS
dc.date.accessioned2026-05-28T15:52:45Z
dc.date.issued1963
dc.description.abstractBesides the emission lines previously identified in Bidelman's catalogue, we have identified Ha and K (Ca II) lines in emission in WY Vel. Furthermore we found that the intensity of the Ca II lines varies.
dc.description.paginacion43 - 44
dc.description.procedenciaLOC
dc.format.discursoNota
dc.format.extent2
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/20203
dc.language.isoInglés
dc.numero.secuencia20200
dc.publisherObservatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
dc.relation.ispartofseriesVol. 2 No. 14
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectNOTE, WY, VELORUM SPECTRUM
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleNOTE ON THE WY VELORUM SAN LUIS POTOSIECTRUM
dc.title.alternativeBOL OBS TONAN TACUB

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