The Alignment Effect at Low Redshift

Details The Alignment Effect at Low Redshift The Alignment Effect at Low Redshift

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...18312206d&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #122.06; Bulletin of the American Astronomical Society, Vol. 25, p.1475

Astronomy and Astrophysics

Astronomy

Scientific paper

Distant radio galaxies (z>1) have spatially extended, multi-component UV (lambda_ {rest} < 4000 Angstroms) continua which are preferentially aligned with the major axis of their associated radio source. Although various physical processes have been suggested to explain this alignment effect, the high-redshift radio galaxies are optically faint and hence discriminating between these processes is very difficult. Therefore, we conducted an optical and near-UV continuum imaging survey of 44 low-redshift radio galaxies (0.08

Affiliated with

Also associated with

No associations

Rating

The Alignment Effect at Low Redshift 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 Alignment Effect at Low Redshift, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Alignment Effect at Low Redshift will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-782125