THE DEVELOPMENT OF SAN LUIS POTOSIIRAL STRUCTURE IN A GALAXY

Simple item page
dc.contributor.authorPISMIS, P
dc.date.accessioned2026-05-28T15:52:05Z
dc.date.issued1962
dc.description.abstractThe main aim of this paper is to show that by postulating the existence of a rotating and shrinking gaseous bulge with a magnetic field as envisaged, and given a rotation curve, a galaxy will have produced and maintained spiral arms during a reasonably lo
dc.description.paginacion127 - 133
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent7
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/19972
dc.language.isoEspañol
dc.numero.secuencia19969
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 3
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectDEVELOPMENT, SPIRAL STRUCTURE, GALAXY
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaGALAXIAS
dc.titleTHE DEVELOPMENT OF SAN LUIS POTOSIIRAL STRUCTURE IN A GALAXY
dc.title.alternativeBOL OBS TONAN TACUB

Files

Collections

Registros completos