THE POLARITIES OF MAGNETIC STARS

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dc.contributor.authorPOVEDA, ARCADIO
dc.date.accessioned2026-05-28T15:49:18Z
dc.date.issued1956
dc.description.abstractThe determination of polarities of magnetic stars is discussed in terms of the classical Zeeman effect, the design of the analyzer for polarized light used, and the appearance of the spectrograms. Is is shown that by a simple inspection of the spectrogram
dc.description.paginacion30 - 32
dc.description.procedenciaLOC
dc.format.discursoArtículo
dc.format.extent3
dc.identifier.issn0082-4879
dc.identifier.urihttps://ahcm.cinvestav.mx/handle/ahcm/19043
dc.language.isoEspañol
dc.numero.secuencia19040
dc.publisherUNAM, Observatorio Astronómico Nacional, CD MEXICO, DF, MEX
dc.relation.ispartofseriesVol. 2 No. 12
dc.source.revistafuenteBOLETIN DE LOS OBSERVATORIOS DE TONANTZINTLA Y TACUBAYA
dc.subjectPOLARITIES, MAGNETIC, STARS
dc.subject.categoriaprincipalASTRONOMIA Y ASTROFISICA
dc.subject.disciplinaCOSMOLOGIA Y COSMOGONIA
dc.subject.subdisciplinaESTRELLAS
dc.titleTHE POLARITIES OF MAGNETIC STARS
dc.title.alternativeBOL OBS TONAN TACUB

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