Interstellar matter and chemical evolution

Details Interstellar matter and chemical evolution Interstellar matter and chemical evolution

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sci...224..345p&link_type=abstract

Science (ISSN 0036-8075), vol. 224, April 27, 1984, p. 345-350.

Astronomy and Astrophysics

Astronomy

6

Abundance, Chemical Evolution, Interstellar Matter, Galactic Evolution, Helium, Hydrogen Clouds, Magellanic Clouds, Nebulae, Oxygen, Spiral Galaxies, Stellar Evolution

Scientific paper

The determination of chemical abundances of the interstellar medium is related to three different areas of astronomy: pregalactic conditions, stellar evolution, and chemical evolution of galaxies. The observed abundances permit the testing of theories associated with these areas. Knowledge of the abundances of helium, carbon, nitrogen, and neon relative to the abundance of hydrogen in the interstellar medium puts limits on current models of cosmology, stellar evolution, and galactic evolution.

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