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When less is more: Are radio galaxies below the Fanaroff-Riley break more polarized on parsec scales?

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dc.contributor.author Kharb, P
dc.contributor.author Shastri, P
dc.contributor.author Gabuzda, D. C
dc.date.accessioned 2006-06-13T11:11:39Z
dc.date.available 2006-06-13T11:11:39Z
dc.date.issued 2005-10-20
dc.identifier.citation Astrophysical Journal, Vol. 632, No. 2, pp. L69–L73 en
dc.identifier.uri http://hdl.handle.net/2248/993
dc.description.abstract We present images showing the first detections of polarizations on parsec scales in the nuclei of four Fanaroof-Riley type I (low-luminosity) radio galaxies. Observations with Very long Baseline Interferomatry at lamda 3.6 cm reveal the presence of ordered magnetic fields within ~1650 Schwarzchild radii of the putative central supermassive black hole. The relatively high fractional polarization in the pc-scale jets of these galaxies is consistent with the standard scheme unifying low-luminosity radio galaxies with BL Lac objects. This result also suggests that these radio galaxies lack the obscuring tori that apparently depolarize the nuclear emission in the more powerful FRII radio galaxies, and that their supermassive blackholes are poorly fed and/or inefficient radiations en
dc.format.extent 564312 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher IOP Publishing
dc.relation.uri http://iopscience.iop.org/1538-4357/632/2/L69
dc.rights © IOP Publishing
dc.subject Galaxies en
dc.subject Active - galaxies: individual (3C 66B, 3C 78, 3C 264, 3C 270) - en
dc.subject Galaxies: magnetic fields en
dc.title When less is more: Are radio galaxies below the Fanaroff-Riley break more polarized on parsec scales? en
dc.type Article en


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