On the abundances of the chemical elements in intergalactic matter

Details On the abundances of the chemical elements in intergalactic matter On the abundances of the chemical elements in intergalactic matter

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....62..255b&link_type=abstract

Astronomy and Astrophysics, vol. 62, no. 1-2, Jan. 1978, p. 255-258. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astronomy

12

Abundance, Astronomical Models, Cosmic Gases, Galactic Evolution, Intergalactic Media, Galactic Clusters, Heavy Elements, Iron, Stellar Evolution, X Ray Astronomy

Scientific paper

A model is proposed for the evolution of S0 galaxies. It consists of a build-up of intergalactic matter via the collisions of galaxies. This is followed by the stripping of galaxies by intergalactic gas so that they remain free from gas. The model is based on star-formation and gas-loss time scales. The model may be used to predict (1) the mass of intergalactic gas, (2) abundances of heavy elements in the intergalactic gas, and (3) abundances of deuterium and secondary nucleosynthesis isotopes in intergalactic matter.

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