DENSITIES POTENCIALS ESCAPE VELOCITIES AND RELATED FUNCTIONS FOR A SAN LUIS POTOSIHERICAL REDUCED GALAXY

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dc.contributor.authorPOVEDA, ARCADIO
dc.contributor.authorOROZCO, I
dc.contributor.authorITURRIA GA, R
dc.date.accessioned2026-05-28T15:50:00Z
dc.date.issued1958
dc.description.abstractThe analysis of stellar motions in a galaxy require a knowledge of several parameters as a function of distance to the center. At present the best table available is the one by de Vaucouleurs, but we feel it is insufficient. In this work we compute the ne
dc.description.paginacion3 - 18
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent15
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/19279
dc.language.isoEspañol
dc.numero.secuencia19276
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 2 No. 2
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectDENSITIES, POTENCIALS, ESCAPE VELOCITIES, RELATED FUNCTIONS, SPHERICAL, REDUCED, GALAXY
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaGALAXIAS
dc.titleDENSITIES POTENCIALS ESCAPE VELOCITIES AND RELATED FUNCTIONS FOR A SAN LUIS POTOSIHERICAL REDUCED GALAXY
dc.title.alternativeBOL OBS TONAN TACUB

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