Protogalactic explosions and intracluster chemical enrichment

Details Protogalactic explosions and intracluster chemical enrichment Protogalactic explosions and intracluster chemical enrichment

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..223d&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 1, Sept. 1980, p. 223-231.

Astronomy and Astrophysics

Astrophysics

3

Abundance, Galactic Clusters, Galactic Evolution, Interstellar Chemistry, Gas Dynamics, Interstellar Gas, Metals

Scientific paper

Using a hydrodynamic model of protogalactic evolution, the amount of iron in rich clusters is explained, deduced from X-ray observations. Calculations show that a strong shock wave originates in the first violent collapse phase and leaves the protogalaxy, carrying out a substantial fraction of its mass, with roughly solar metallicity and high temperature. It is also shown that hot material ejected from proto-cD galaxies can probably explain the observed X-ray emission in clusters.

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