NEW FLARE STARS AND THE SAN LUIS POTOSIECTRUM RATE OF VARIATION RELATION

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dc.contributor.authorHARO, G
dc.contributor.authorCHAVIRA, E
dc.date.accessioned2026-05-28T15:49:18Z
dc.date.issued1956
dc.description.abstractIn this study we confirm that whenever there is a group of T Tauri stars, there is the possibility of finding, associated to them, rapid variables. We have thus found 7 new variables of the UV Ceti Type in the Taurus dark region. From the new data we can
dc.description.paginacion3 - 16
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent13
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/19047
dc.language.isoEspañol
dc.numero.secuencia19044
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 2 No. 12
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectNEW, FLARE, STARS, SPECTRUM, RATE, VARIATION RELATION
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleNEW FLARE STARS AND THE SAN LUIS POTOSIECTRUM RATE OF VARIATION RELATION
dc.title.alternativeBOL OBS TONAN TACUB

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