The parsec-scale central components of FR I radio galaxies

Details The parsec-scale central components of FR I radio galaxies The parsec-scale central components of FR I radio galaxies

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..205...74k&link_type=abstract

Galaxies and their Constituents at the Highest Angular Resolutions, Proceedings of IAU Symposium #205, held 15-18 August 2000 at

Computer Science

Scientific paper

A majority of a complete sample of 3CR FR I radio galaxies show unresolved optical nuclear sources on the scales of 0.1 arcsec. These Compact Central Cores (CCC) have been interpreted as the optical counterparts of the non-thermal radio cores in these radio galaxies (Chiaberge et al. 1999). We show that the optical flux density of these CCCs is correlated with the radio core prominence. This correlation supports the argument of Chiaberge et al. that the CCC radiation is of a non-thermal synchrotron origin, which is relativistically beamed along with the radio emission.

Affiliated with

Also associated with

No associations

Rating

The parsec-scale central components of FR I radio galaxies 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 parsec-scale central components of FR I radio galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The parsec-scale central components of FR I radio galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1362869