Chemical evolution of galaxies and abundances in low-mass stars

Details Chemical evolution of galaxies and abundances in low-mass stars Chemical evolution of galaxies and abundances in low-mass stars

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987japa....8..147a&link_type=abstract

(IAU, Meeting on Nucleosynthesis in the Galaxy from the Study of Low-mass Stars, New Delhi, India, Nov. 27, 1985) Journal of Ast

Astronomy and Astrophysics

Astrophysics

5

Abundance, Chemical Evolution, Galactic Evolution, Stellar Composition, Gas Density, Nuclear Fusion, Star Formation Rate, Stellar Mass

Scientific paper

It is noted that low-mass stars can be used to determine the metallicity at the beginning of galactic evolution and to provide a better understanding of the formation and evolution of many nuclear species. The main parameters governing the evolution of galaxies are considered, including the rate of star formation, the stellar initial mass function, and the nuclear yields. A list of the nuclear species which should be observed in low-mass stars in order to progress in the analysis of such evolution is provided. It is concluded that low-mass stars should constrain the choice of the parameters governing the chemical evolution of galaxies.

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