21 centimeter observations of supercluster galaxies - The bridge between Coma and A1367

Details 21 centimeter observations of supercluster galaxies - The bridge between Coma and A1367 21 centimeter observations of supercluster galaxies - The bridge between Coma and A1367

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...269...13c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 269, June 1, 1983, p. 13-28.

Astronomy and Astrophysics

Astronomy

40

Centimeter Waves, Galactic Clusters, Galactic Evolution, Interstellar Gas, Radio Astronomy, Hydrogen, Spiral Galaxies, X Ray Astronomy

Scientific paper

The authors present 21 cm observations of galaxies in the region of the Coma-A1367 supercluster. It is shown that galaxies near the cluster center are hydrogen deficient while galaxies which are in between the two clusters have a normal hydrogen content. A crossing time of about 1.7×109 yr is defined by the radius of the region of transition between deficient and nondeficient galaxies and the cluster's velocity dispersion. The gas removed by stripping is a small fraction of the gas observed in the X-ray region.

Affiliated with

Also associated with

No associations

Rating

21 centimeter observations of supercluster galaxies - The bridge between Coma and A1367 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 21 centimeter observations of supercluster galaxies - The bridge between Coma and A1367, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 21 centimeter observations of supercluster galaxies - The bridge between Coma and A1367 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1504620