The evolution of galaxies in clusters. I - ISIT photometry of C1 0024+1654 and 3C 295

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

591

Astronomical Photometry, Galactic Clusters, Galactic Evolution, Galactic Structure, Graphs (Charts), Reference Stars, Spiral Galaxies, Tables (Data), Vidicons

Scientific paper

A description is presented of a project of two-color photometry of a number of distant clusters. The KPNO ISIT vidicon described by Lynds (1975) and Strom (1976) is used in the project. The first results reported are related to photometry studies of the two rich clusters, C1 0024+1654 (z = 0.39) and the cluster around 3C 295 (z = 0.46). It is shown that between one third and one half of the galaxies in C1 0024+1654 and the cluster around 3C 295 have the colors of spirals. If they are spirals, this population is similar to those of nearby spiral-rich clusters like the Hercules cluster (Oemler, 1974). Structurally, however, these clusters resemble, not clusters like Hercules, which are irregular and lack central concentration, but rather Coma and other cD clusters. It appears, therefore, that the dependence of content on form, which nearby clusters show, is not shown by these distant clusters observed at an earlier epoch.

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

The evolution of galaxies in clusters. I - ISIT photometry of C1 0024+1654 and 3C 295 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 evolution of galaxies in clusters. I - ISIT photometry of C1 0024+1654 and 3C 295, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolution of galaxies in clusters. I - ISIT photometry of C1 0024+1654 and 3C 295 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-943070

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