RUNAWAY STARS AS THE RESULT OF THE GRAVITATIONAL COLLAPSE OF PROTOSTELLAR CLUSTERS

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dc.contributor.authorRUIZ, J
dc.contributor.authorPOVEDA, ARCADIO
dc.contributor.authorALLEN, CHARLES GRANT
dc.date.accessioned2026-05-28T16:29:09Z
dc.date.issued1969
dc.description.abstractSome of the difficulties in our present understanding of the origin of run-away stars and expanding clusters are briefly discussed; an alternative explanation for these phenomena is proposed here as the result of dynamical interactions during the collapse
dc.description.paginacion86 - 90
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent5
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22310
dc.language.isoInglés
dc.numero.secuencia22307
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectRESULT, GRAVITATIONAL COLLAPSE, PROTO, STELLAR CLUSTERS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleRUNAWAY STARS AS THE RESULT OF THE GRAVITATIONAL COLLAPSE OF PROTOSTELLAR CLUSTERS
dc.title.alternativeBOL OBS TONAN TACUB

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