Hot gas in galactic clusters

Details Hot gas in galactic clusters Hot gas in galactic clusters

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991s%26w....30..159t&link_type=abstract

Sterne und Weltraum (ISSN 0039-1263), vol. 30, March 1991, p. 159-163. In German.

Astronomy and Astrophysics

Astrophysics

Galactic Clusters, High Temperature Gases, Intergalactic Media, Interstellar Gas, Chemical Evolution, Cooling Flows (Astrophysics), Stellar Winds

Scientific paper

The characteristics, origin, and evolution of hot gas in galactic clusters are discussed. The contributions of stellar winds, supernova explosions, intergalactic interactions, and ram pressure from galactic movements to the production of the gas are addressed. The role of cooling flows in the evolution of the gas is considered. The information on the dynamic state and chemical evolution of galactic structures provided by the distribution of the gas is examined.

Affiliated with

Also associated with

No associations

Rating

Hot gas in galactic 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 Hot gas in galactic clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hot gas in galactic clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-939038