A NEW SLOWFLARE STAR IN ORION

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dc.contributor.authorPARSAMIAN, E
dc.contributor.authorHARO, G
dc.date.accessioned2026-05-28T16:29:10Z
dc.date.issued1969
dc.description.abstractPhotometric and spectroscopic characteristics are defined of the "slow" and "fast" flare stars. A new case of a "slow" flare star in Orion, is presented. It showed an increase of > 8.4 magnitudes in UV, during a period of 118 minutes. The peculiar physica
dc.description.paginacion45 - 53
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent8
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22320
dc.language.isoInglés
dc.numero.secuencia22317
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.publisherObservatorio Astrofísico de Tonantzintla, Pue, Pue, Mex
dc.relation.ispartofseriesVol. 5
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectNEW, SLOWFLARE, STAR, ORION
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleA NEW SLOWFLARE STAR IN ORION
dc.title.alternativeBOL OBS TONAN TACUB

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