THE MASSES OF SAN LUIS POTOSIHERICAL GALAXIES M32 A LIKELY APPLICATION

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dc.contributor.authorPOVEDA, ARCADIO
dc.date.accessioned2026-05-28T15:50:00Z
dc.date.issued1958
dc.description.abstractOur knowledge of the mass of early E galaxies is very limited. We propose that it is safer to estimate the mass of a spherical galaxy from the dispersion of its star velocities as determined by Minkowski for M32, and we analize the method with the help of
dc.description.paginacion3 - 7
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent4
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/19280
dc.language.isoEspañol
dc.numero.secuencia19277
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 2 No. 17
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectMASSES, SPHERICAL, GALAXIES, LIKELY APPLICATION
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleTHE MASSES OF SAN LUIS POTOSIHERICAL GALAXIES M32 A LIKELY APPLICATION
dc.title.alternativeBOL OBS TONAN TACUB

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