A study of 4C 13.66 - the final identification and redshift for the revised 3C sample

Details A study of 4C 13.66 - the final identification and redshift for the revised 3C sample A study of 4C 13.66 - the final identification and redshift for the revised 3C sample

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.279l..13r&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 279, Issue 1, pp. L13-L20.

Astronomy and Astrophysics

Astronomy

9

Galaxies: Active, Galaxies: Individual: 4C 13.66, Infrared: Galaxies, Radio Continuum: Galaxies

Scientific paper

We use new optical and near-infrared data to identify the radio source 4C 13.66 with a K=18.2 galaxy at z=1.45, and use new radio images to study its relatively unusual radio structure. Prior to this work 4C 13.66 was the only radio source out of 173 in the revised 3C sample of Laing, Riley & Longair without a spectroscopic redshift. We discuss the vital role of near-infrared spectroscopy in securing the final redshift for this sample.

Affiliated with

Also associated with

No associations

Rating

A study of 4C 13.66 - the final identification and redshift for the revised 3C 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 A study of 4C 13.66 - the final identification and redshift for the revised 3C sample, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A study of 4C 13.66 - the final identification and redshift for the revised 3C sample will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1615841