THE HR DIAGRAMS OF YOUNG CLUSTERS AND THE FORMATION OF PLANETARY SYSTEMS

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dc.contributor.authorPOVEDA, ARCADIO
dc.date.accessioned2026-05-28T15:58:09Z
dc.date.issued1968
dc.description.abstractThe existence of T Tauri and flare stars located below the main sequence in some young clusters pose a difficult problem of interpretation for gravitational contraction within conventional stellar theory. We introduce the hypotheses that when solar type p
dc.description.paginacion15 - 21
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent7
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/21956
dc.language.isoEspañol
dc.numero.secuencia21953
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectDIAGRAMs, YOUNG CLUSTERS, FORMATION, PLANETARY SYSTEMS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaASTRONOMIA OPTICA
dc.subject.subdisciplinaATMOSFERA PLANETARIA
dc.titleTHE HR DIAGRAMS OF YOUNG CLUSTERS AND THE FORMATION OF PLANETARY SYSTEMS
dc.title.alternativeBOL OBS TONAN TACUB

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