THE CONTINUUM EMISSION OF THE ORION NEBULA

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dc.contributor.authorMENDEZ, ME
dc.date.accessioned2026-05-28T15:54:55Z
dc.date.issued1965
dc.description.abstractThe continuum produced by the brightest region of the Orion Nebula has been observed photoelectrically. The spectral range covered is from ?~3500 to ?~11000. The various processes contributing to the continuum energy have been studied. The component provi
dc.description.paginacion41 - 48
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent8
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/20856
dc.language.isoInglés
dc.numero.secuencia20853
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectCONTINUUM EMISSION, ORION NEBULA
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleTHE CONTINUUM EMISSION OF THE ORION NEBULA
dc.title.alternativeBOL OBS TONAN TACUB

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