Gigahertz-Peaked Spectrum Radio Sources

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

9 pages, to appear in "Radio Astronomy at the Fringe"; a conference held in Green Bank, WV in honor of Ken Kellermann's 65th b

Scientific paper

The study of compact active galactic nuclei (AGN) that possess convex radio spectra (the gigahertz-peaked spectrum radio sources) offers a unique opportunity to probe both the early evolutionary stages of relativistic AGN jets and their immediate nuclear environments. In this article I trace Ken Kellermann's early investigations of these sources, which played a major role in justifying the development of modern-day VLBI techniques. I describe how our understanding of these AGN has progressed since Kellermann's early discoveries, and discuss several ways in which the current classification scheme can be simplified to reflect intrinsic source characteristics, rather than observer-biased quantities. Finally, I discuss recent results from the VLBA 2 cm survey concerning the relativistic jet kinematics of the two-sided peaked-spectrum sources 4C +12.50 (PKS 1345+125) and OQ 208 (1404+286).

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

Gigahertz-Peaked Spectrum Radio Sources 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 Gigahertz-Peaked Spectrum Radio Sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gigahertz-Peaked Spectrum Radio Sources will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-534827

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