On a possible metallicity gradient in SMR stars

Details On a possible metallicity gradient in SMR stars On a possible metallicity gradient in SMR stars

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987japa....8..141c&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

7

Dwarf Stars, Metallic Stars, Stellar Composition, Subgiant Stars, Abundance, Astronomical Catalogs, Hertzsprung-Russell Diagram, Hydrogen, Iron

Scientific paper

The possibility of existence of a metallicity gradient in
supermetal-rich (SMR) stars is discussed. It is concluded that the SMR
phenomenon was more active in the past than it is now.

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