RAPID VARIABLES IN THE ORION NEBULA

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dc.contributor.authorRIVERA TERRAZAS, LUIS
dc.contributor.authorHARO, G
dc.date.accessioned2026-05-28T15:50:48Z
dc.date.issued1960
dc.description.abstractDuring a study of the Ha emission stars in and near the Orion nebula Haro found a good number of cases where the Haemission line or the continuum varies in intensity strongly suggesting a "Flare" star. As a continuation of this work we have found 7 new st
dc.description.paginacion3 - 15
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent12
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/19579
dc.language.isoEspañol
dc.numero.secuencia19576
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 1 No. 10
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectRAPID, VARIABLES, ORION NEBULA
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleRAPID VARIABLES IN THE ORION NEBULA
dc.title.alternativeBOL OBS TONAN TACUB

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