ON THE RECESSION OF THE STELLAR ASSOCIATIONS FROM THE GALACTIC CENTER

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dc.contributor.authorPISMIS, P
dc.date.accessioned2026-05-28T15:48:44Z
dc.date.issued1955
dc.description.abstract21-cm studies have shown that at about 3kpc from the galactic center a neutral hydrogen arm is expanding at the rate of 50 km/s. We have studied the recession of stellar associations from the galactic center since these objects, are presumably recent form
dc.description.paginacion3 - 6
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent4
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/18957
dc.language.isoEspañol
dc.numero.secuencia18954
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 2 No. 19
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectRECESSION, STELLAR, ASSOCIATION, GALACTIC CENTER
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleON THE RECESSION OF THE STELLAR ASSOCIATIONS FROM THE GALACTIC CENTER
dc.title.alternativeBOL OBS TONAN TACUB

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