Clustering around radio galaxies at z~1.5

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

LaTeX, 6 pages, Elsevier Science format. To appear in "Radio galaxies: past, present & future". eds. M. Jarvis et al., Leiden,

Scientific paper

10.1016/S1387-6473(03)00044-7

The importance of studying old elliptical galaxies at redshift z ~ 1.5 is reviewed, considering both what can be learned by extending studies of the evolution of cluster galaxy scaling relations to earlier cosmic epochs, and the age-dating of old elliptical galaxies at high redshifts. Following this, the first results are provided of an on-going project to find such distant elliptical galaxies, through an investigation of the cluster environments of powerful radio sources with redshifts 1.44 < z < 1.7. These studies show a considerable excess of red galaxies in the radio sources fields, with the magnitudes (K >~ 17.5) and colours (R-K > 4) expected of old passively evolving galaxies at the radio source redshift. The red galaxy overdensities are found on two different scales around the radio sources; a pronounced small-scale peak at radial distances of <~ 150 kpc, and a weaker large-scale excess extending out to 1 - 1.5 Mpc. The presence and richness of these red galaxy excesses varies considerably from source to source. An interpretation of these results is provided.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Clustering around radio galaxies at z~1.5 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 Clustering around radio galaxies at z~1.5, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clustering around radio galaxies at z~1.5 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-86270

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.