ON THE WAVY NATURE OF ROTATION CURVES IN THE GALAXIES

dc.contributor.authorPISMIS, P
dc.date.accessioned2026-05-28T16:29:09Z
dc.date.issued1969
dc.description.abstractIn this work we call attention to the variation of the "waves" in the rotation curves of spiral galaxies, argue in favor of their physical reality and attempt an interpretation of them. As a specific case NGC 4258 is analyzed.
dc.description.paginacion8 - 14
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent7
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/22309
dc.language.isoInglés
dc.numero.secuencia22306
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectWAVY, NATURE, ROTATION, CURVES, GALAXIES
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaGALAXIAS
dc.titleON THE WAVY NATURE OF ROTATION CURVES IN THE GALAXIES
dc.title.alternativeBOL OBS TONAN TACUB

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