BD 11522 HV 11110 A POSSIBLE FLARE STAR OF TYPE K2

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dc.contributor.authorMUNCH, LUIS
dc.contributor.authorMUNCH, G
dc.date.accessioned2026-05-28T15:50:26Z
dc.date.issued1959
dc.description.abstractUnusually strong emission lines for a late type dwarf were noted for the star BD+1° 1522. It was also found to have variations in its spectrum we are inclined to consider it as a flare star that underwent during one of our exposures a sudden increase in b
dc.description.paginacion36 - 38
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent3
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/19419
dc.language.isoEspañol
dc.numero.secuencia19416
dc.publisherObservatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
dc.relation.ispartofseriesVol. 2 No. 13
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectPOSSIBLE, FLARE, STAR, TYPE K2
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleBD 11522 HV 11110 A POSSIBLE FLARE STAR OF TYPE K2
dc.title.alternativeBOL OBS TONAN TACUB

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