Parsec Scale Properties of Brightest Cluster Galaxies

Details Parsec Scale Properties of Brightest Cluster Galaxies Parsec Scale Properties of Brightest Cluster Galaxies

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..402..163g&link_type=abstract

Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technologies ASP Conference Series, Vol. 402, proceedings o

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We present new VLBI observations of Brightest Cluster Galaxies in eight nearby Abell clusters. These data show a possible difference between Brightest Cluster Galaxies in cool core clusters (two-sided pc scale jets) and in non cool core clusters (one-sided pc scale jets). We suggest that this difference could be due to the jet interaction with the surrounding medium. More data are necessary to discuss if pc-scale properties of Brightest Cluster Galaxies are influenced by their peculiar morphology and position in the center of rich clusters of galaxies.

Affiliated with

Also associated with

No associations

Rating

Parsec Scale Properties of Brightest Cluster 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 Parsec Scale Properties of Brightest Cluster Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Parsec Scale Properties of Brightest Cluster Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-818262