RADIAL VELOCITIES OF SUPERGIANTS STARS AROUND THE H AND X PERSEI CLUSTER

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dc.contributor.authorMENDOZA, EUGENIO
dc.contributor.authorCHAVIRA, E
dc.date.accessioned2026-05-28T15:48:14Z
dc.date.issued1953
dc.description.abstractRadial velocities of seven supergiant early-type stars probable members of the h and X Persei cluster have been derived from spectrograms taken at the Mc Donald Observatory. The possibility to verify with these velocities and eighteen other obtained from
dc.description.paginacion1 - 10
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent10
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/18757
dc.language.isoEspañol
dc.numero.secuencia18754
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 1 No. 3
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectRADIAL VELOCITIES, SUPERGIANTS, STARS, AROUND, H, X, PERSEI CLUSTER
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleRADIAL VELOCITIES OF SUPERGIANTS STARS AROUND THE H AND X PERSEI CLUSTER
dc.title.alternativeBOL OBS TONAN TACUB

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