BE AND AE STARS IN PERSEUS AND CASSIOPEA

dc.contributor.authorGONZALEZ, G
dc.contributor.authorGONZALEZ, G
dc.date.accessioned2026-05-28T15:48:28Z
dc.date.issued1954
dc.description.abstractAn area of 179 square degrees lying approximately between l=90° to 103° and b=+4° to -7° has been searched with the purpose of finding early-type stars with Ha in emission and with photographic magnitudes as faint as 14.5m. During our presente work we hav
dc.description.paginacion3 - 20
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent17
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/18851
dc.language.isoEspañol
dc.numero.secuencia18848
dc.publisherObservatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
dc.relation.ispartofseriesVol. 1 No. 9
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectSTARS, PERSEUS, CASSIOPEA
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleBE AND AE STARS IN PERSEUS AND CASSIOPEA
dc.title.alternativeBOL OBS TONAN TACUB

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