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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2677
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dc.contributor.authorBhatt, H. C-
dc.contributor.authorJain, S. K-
dc.date.accessioned2008-07-14T09:08:53Z-
dc.date.available2008-07-14T09:08:53Z-
dc.date.issued1993-09-
dc.identifier.citationAstronomy and Astrophysics , Vol. 276, No. 2, pp. 507 - 510en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/2677-
dc.description.abstractOptical linear polarization measurements for stars in the regions of the molecular clouds B 227 and L 121 are presented. The magnetic field geometry in the clouds as indicated by the polarization maps is discussed in relation to their morphology. In the outer parts of B 227 the field is more or less parallel to the long axis of the cloud while in L 121 it appears to be parallel to the short axis. The wavelength dependence of polarization for two stars in the region of B 227 is found to be anomalous.en
dc.format.extent514452 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993A%26A...276..507Ben
dc.subjectPolarizationen
dc.subjectInterstellar mediumen
dc.subjectMolecular cloudsen
dc.subjectMagnetic fieldsen
dc.titlePolarization Maps for the Dark Clouds B:227 and L:121en
dc.typeArticleen
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