Old disk subdwarfs

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Hertzsprung-Russell Diagram, M Stars, Stellar Evolution, Stellar Structure, Subdwarf Stars, Late Stars, Main Sequence Stars, Photometry

Scientific paper

Measurements of CaH and TiO band strengths are presented for M dwarfs of
the old disk population which lie below the main sequence. Their band
strengths imply a composition intermediate between that of halo
subdwarfs and that of disk dwarfs.

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