ON THE THERMAL RADIO EMISSION OF THE CYGNUS LOOP

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dc.contributor.authorPOVEDA, ARCADIO
dc.date.accessioned2026-05-28T15:56:58Z
dc.date.issued1967
dc.description.abstractA model of supernova remnants of Type II inspired only by the optical evidence implies a thermal radio emission which is in accord with current measurement of the flux density from the Cygnus Loop and that, therefore, its radio flux is mostly thermal at 1
dc.description.paginacion49 - 50
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent2
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/21562
dc.language.isoInglés
dc.numero.secuencia21559
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectTHERMAL, RADIO EMISSION, CYGNUS LOOP
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaASTRONOMIA OPTICA
dc.subject.subdisciplinaASTRONOMIA DE POSICION
dc.titleON THE THERMAL RADIO EMISSION OF THE CYGNUS LOOP
dc.title.alternativeBOL OBS TONAN TACUB

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