Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..558..721b&link_type=abstract
HIGH ENERGY GAMMA-RAY ASTRONOMY: International Symposium. AIP Conference Proceedings, Volume 558, pp. 721-724 (2001).
Astronomy and Astrophysics
Astronomy
9
Active And Peculiar Galaxies And Related Systems, Radio, Microwave
Scientific paper
We present first results from the analysis of multi-epoch VLBI observations of the EGRET detected sources [9] in the CJ-F sample (Caltech Jodrell-Flat-spectrum, [10]). These objects form a subsample of 14 sources within the 293 AGN of the full CJ-F sample. 5 GHz VLBI snapshot observations of the CJ-F sources are continuously being performed in order to create a valid database for thorough statistical tests of pc-scale jet motion in AGN. All gamma-bright CJ-F AGN have been observed at least twice with the VLBA, which enables us to investigate jet component motions and paths. In particular, we concentrate on the analysis of those properties supposed to be essential for gamma-ray production, i.e., superluminal motion and bending. A paper discussing the possible relation between morphological changes and gamma-ray flaring/production is in preparation. .
Britzen Silke
Browne Ian W.
Campbell Robert Moses
Pearson Timothy. J.
Readhead Anthony C. S.
No associations
LandOfFree
The properties of the gamma-ray blazars in the CJ-F VLBI sample 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 The properties of the gamma-ray blazars in the CJ-F VLBI sample, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The properties of the gamma-ray blazars in the CJ-F VLBI sample will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1182665