Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...233..427r&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 233, no. 2, July 1990, p. 427-436.
Astronomy and Astrophysics
Astrophysics
11
Astronomical Spectroscopy, Galactic Evolution, Iron, Metallicity, Milky Way Galaxy, Supernova Remnants, Astronomical Models, Supernovae, Wolf-Rayet Stars
Scientific paper
The chemical evolution of various Galactic elements is determined. The
calculations are shown to be consistent with the IMF and star formation
rate used to model the spectrophotometric evolution of Sc galaxies. The
abundance of iron relative to the other elements is studied in detail
and explanations are provided.
Rocca-Volmerange Brigitte
Schaeffer Richard
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