The halo population G and K subdwarfs

Details The halo population G and K subdwarfs The halo population G and K subdwarfs

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.104..219s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 104, no. 2, Sept. 1984, p. 219-223.

Astronomy and Astrophysics

Astrophysics

1

Metallicity, Subdwarf Stars, Interstellar Extinction, Line Spectra, Spectral Energy Distribution, Spectrum Analysis, Stellar Spectrophotometry

Scientific paper

The photometry of G and K subdwarfs is analyzed in order to determine their metallicity using a system invented by the Lithuanian Academy of Sciences (the Vilnius method). The Vilnius method permits the recognition of F-G-K subdwarfs in conditions of interstellar reddening. For quantitative interpretation of line strengths, a group of synthetic spectrum calculations were used. A series of diagrams is provided which illustrates the photometric data.

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