THE DETECTION OF QUARKS IN DIFFUSE NEBULAE

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dc.contributor.authorMENDEZ, ME
dc.contributor.authorCARRASCO, L
dc.date.accessioned2026-05-28T16:31:14Z
dc.date.issued1971
dc.description.abstractThe problem of detecting quarks in diffuse nebulae is studied, considering the existence of hydrogenic quark atoms. It is shown that the predicted upper limit of abundance, relative to hydrogen, is 1.5 X 10^8 if tne infrared lines produced by the quark at
dc.description.paginacion54 - 56
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent2
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/23134
dc.language.isoInglés
dc.numero.secuencia23131
dc.publisherUNAM, Instituto de Astronomía, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 5
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectDETECTION, QUARKS, DIFFUSE NEBULAE
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleTHE DETECTION OF QUARKS IN DIFFUSE NEBULAE
dc.title.alternativeBOL OBS TONAN TACUB

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