AN INTERPRETATION OF THE CHANGES OBSERVED IN V1057 CYGNI

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dc.contributor.authorPISMIS, P
dc.date.accessioned2026-05-28T16:32:39Z
dc.date.issued1972
dc.description.abstractIt is argued that the brightening of V1057 Cygni, a T-Tauri star, roughly from photographic magnitude 15.5 to 10.0 and its change of spectral type from about KO to A1, at which the star appears to remain, may be explained by a fast readjustment of mass di
dc.description.paginacion131 - 133
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent3
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/23648
dc.language.isoInglés
dc.numero.secuencia23645
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 6
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectINTERPRETATION, CHANGES, OBSERVED
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleAN INTERPRETATION OF THE CHANGES OBSERVED IN V1057 CYGNI
dc.title.alternativeBOL OBS TONAN TACUB

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