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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2841
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dc.contributor.authorKharb, P-
dc.contributor.authorGabuzda, D-
dc.contributor.authorShastri, P-
dc.date.accessioned2008-07-23T09:55:39Z-
dc.date.available2008-07-23T09:55:39Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 761 - 764en
dc.identifier.urihttp://hdl.handle.net/2248/2841-
dc.description.abstractWe present results of the VLBA3 polarization observations of "X-ray selected" BL Lac objects from the HEAO-l survey and also a few from the ROSAT-Green Bank (RGB) sample. These primarily high energy peaked BL Lacs (HBLs) have "core-jet" morphologies with modestly polarized pc-scale cores and jet components, similar to their radio-selected counterparts (primarily low energy peaked BL Lacs, LBLs). However, we find that the jets in HBLs show preferentially longitudinal magnetic fields, as opposed to the jets in LBLs, which tend to have transverse magnetic fields.en
dc.format.extent170852 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectBL Lacertae Objects-Galaxiesen
dc.subjectActive Radio Galaxiesen
dc.titlePolarization study of BL Lacertae objects on pc-scalesen
dc.typeArticleen
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