Asymmetry of jets, lobe length and spectral index in quasars

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

to be published in MNRAS. 12 pages, uses mn.sty. Replacement corrects for error in postscript (fig. 1)

Scientific paper

The less depolarized lobe of a radio source is generally the lobe containing the jet (Laing-Garrington correlation) but the less depolarized lobe is also generally that with the flatter radio spectrum (Liu-Pooley correlation). Both effects are strong; taken together they would imply a correlation between jet side and lobe spectral index, i.e. between an orientation-dependent feature and one which is intrinsic. We test this prediction using detailed spectral imaging of a sample of quasars with well-defined jets and investigate whether the result can be reconciled with the standard interpretation of one-sided jets in terms of relativistic aberration. Our central finding is that the spectrum of high surface brightness regions is indeed flatter on the jet side, but that the spectrum of low surface brightness regions is flatter on the side with the longer lobe. We discuss possible causes for these correlations and favour explanations in terms of relativistic bulk motion in the high surface brightness regions and differential synchrotron ageing in the extended lobe material.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Asymmetry of jets, lobe length and spectral index in quasars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Asymmetry of jets, lobe length and spectral index in quasars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Asymmetry of jets, lobe length and spectral index in quasars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-331808

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.