An introduction to chemical evolution of the Galaxy based on the metal-poor stars

Details An introduction to chemical evolution of the Galaxy based on the metal-poor stars An introduction to chemical evolution of the Galaxy based on the metal-poor stars

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..315t&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 6, p. 315 - 320 (2003)

Astronomy and Astrophysics

Astronomy

Galaxy, Chemical Evolution, Metal-Poor Stars

Scientific paper

Studies of chemical evolution and formation of the Galaxy have been carried out based on spectroscopic observations of metal-poor stars. In recent years, much fainter, extremely metal-poor stars have been observed with 8-10 m class telescopes, while the observations of rather bright and moderately metal-poor stars are also important. An introductory explanation is given about the studies of the chemical evolution of the Galaxy using OAO 188 cm + HIDES.

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