Neutral hydrogen in A 2052 and other cooling flow clusters

Details Neutral hydrogen in A 2052 and other cooling flow clusters Neutral hydrogen in A 2052 and other cooling flow clusters

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...250...67j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 250, no. 1, Oct. 1991, p. 67-69.

Astronomy and Astrophysics

Astrophysics

13

Active Galaxies, Cooling Flows (Astrophysics), Galactic Clusters, H I Regions, Radio Galaxies, Centimeter Waves, Hydrogen Atoms, Neutral Atoms

Scientific paper

New upper limits on H I absorption and emission near the radio source 3 C 317 in the cooling flow cluster A 2052 are reported. Considering published H I data on radio galaxies in cooling flows, a probable anticorrelation between radio power and observed absorption is noted. Clusters where absorption but no emission is observed allow estimates of the spatial extent (about 20 kpc) and spin temperature (about 100 K) of the absorbing regions.

Affiliated with

Also associated with

No associations

Rating

Neutral hydrogen in A 2052 and other cooling flow clusters 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 Neutral hydrogen in A 2052 and other cooling flow clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutral hydrogen in A 2052 and other cooling flow clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1874523