ON A DUST RICH REGION OF THE ORION NEBULA

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dc.contributor.authorMENDEZ, ME
dc.date.accessioned2026-05-28T15:54:55Z
dc.date.issued1965
dc.description.abstractA region in the vicinity of Theta 2 Ori is studied to try to explain the differences in appearance between images below 3650 Å, and those at 5200 A. And it is concluded that there is an appreciable amount of dust close to the star.
dc.description.paginacion104 - 105
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent2
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/20847
dc.language.isoInglés
dc.numero.secuencia20844
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 4
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectRICH, REGION, ORION NEBULA
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleON A DUST RICH REGION OF THE ORION NEBULA
dc.title.alternativeBOL OBS TONAN TACUB

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