Open AccessA Millimetre/Submillimetre Polarization Survey of Compact Flat‐Spectrum Radio Sources
Author(s) -
Nartallo R.,
Gear W. K.,
Murray A. G.,
Robson E. I.,
Hough J. H.
Publication year - 1998
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.1998.01405.x
Subject(s) - physics , millimeter , astrophysics , polarization (electrochemistry) , quasar , wavelength , magnetic field , jet (fluid) , shock wave , shock (circulatory) , computational physics , optics , galaxy , mechanics , chemistry , quantum mechanics , medicine
We present the results of the first survey and monitoring study of the linear polarization properties of compact, flat‐spectrum radio sources at mm/submm wavelengths and discuss the implications of the inferred magnetic field structure for the emission models involving shock waves in relativistic jets on subparsec scales. We find significant polarization in most sources but, in general, the magnetic field on subparsec scales is less well ordered than on parsec scales. We observe no difference in polarization properties between the BL Lac objects and compact flat‐spectrum quasars at these wavelengths. Although we find the behaviour of some sources, particularly the most highly polarized, to be very consistent with the predictions of transverse shock‐in‐jet models, the detailed behaviour of most objects is not. Conical shock structures can more readily explain the observed diverse behaviour of the sample, although some degree of bending of the jet may still be necessary in some cases.