Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2632
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dc.contributor.authorJain, S. K-
dc.contributor.authorBhatt, H. C-
dc.date.accessioned2008-07-11T06:52:29Z-
dc.date.available2008-07-11T06:52:29Z-
dc.date.issued1995-06-
dc.identifier.citationAstronomy and Astrophysics Supplement Series, Vol.111, No. 3, pp. 399 - 405en
dc.identifier.issn0365-0138-
dc.identifier.urihttp://hdl.handle.net/2248/2632-
dc.description.abstractWe report our measurements of linear polarization of a number of Herbig Ae/Be stars made at several epochs during the period 1989-1993. These results together with the observations compiled from the published sources have been analysed to study the variability of polarization in Herbig Ae/Be stars. It is found that polarimetric variability is a common feature of this class of objects. Most of the objects are variable on time scales >=1yr. Some objects have shown large variations on time scales as short as ~1 month indicating structural changes in the distribution of circumstellar matter close to the star within a few tens of stellar radii. Variations in the polarization position angle are not always correlated with variations in the degree of polarization.en
dc.format.extent863873 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1995A%26AS..111..399Jen
dc.subjectStars: Emission-Lineen
dc.subjectAEen
dc.subjectPolarizationen
dc.subjectStars: Variableen
dc.subjectStars: Pre-Main-Sequenceen
dc.titleStudy of variability of the polarization in Herbig Ae/Be starsen
dc.typeArticleen
Appears in Collections:IIAP Publications

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