OPTICAL STUDY OF THE GALAXY M101 DERIVATION OF A MASS MODEL FROM THE KINEMATIC OF THE GAS

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dc.contributor.authorROSADO, A
dc.contributor.authorMONNIER, MARCEL
dc.contributor.authorCOMTE, G
dc.date.accessioned2026-05-28T16:56:47Z
dc.date.issued1979
dc.description.paginacion73 - 81
dc.description.procedenciaEXT
dc.format.discursoArtículo
dc.format.extent9
dc.identifier.issn0004-6361
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/30481
dc.language.isoInglés
dc.numero.secuencia30478
dc.publisherOBSERV HAUTE PROVENCE,PARIS,FRANCE
dc.publisherOBSERV LYON,LYON,FRANCE
dc.publisherUNIV NACL AUTONOMA MEXICO,INST ASTRON,MEXICO CITY 20,MEXICO
dc.relation.ispartofseriesVol. 72
dc.source.revistafuenteASTRONOMY & ASTROPHYSICS
dc.subjectOPTICAL STUDY, GALAXY, DERIVATION, MODEL, KINEMATIC, GAS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaGALAXIAS
dc.titleOPTICAL STUDY OF THE GALAXY M101 DERIVATION OF A MASS MODEL FROM THE KINEMATIC OF THE GAS
dc.title.alternativeASTROPHYS J

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