The near-IR NA I doublet and CA II triplet in late-type stars and the determination of stellar atmosphere parameters

Astronomy and Astrophysics – Astrophysics

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Giant Stars, Late Stars, Metallicity, Spectral Line Width, Stellar Atmospheres, Stellar Spectra, Calcium, Charge Coupled Devices, Near Infrared Radiation, Sodium, Stellar Composition, Stellar Gravitation, Stellar Spectrophotometry

Scientific paper

CCD spectroscopic observations in the near-IR (7990-8680 A) for a sample of 144 late type stars are presented. The dependence of the Na I doublet (8183 and 8194 A) and the Ca II triplet (8498, 8542 and 8662 A) on stellar atmospheric parameters is investigated. It is confirmed in stars of spectral types later than G0 a dependence of line strength on effective temperature, surface gravity, and metallicity in good agreement with previous studies. However, the present sample contains many more very late type stars than previous studies, and these stars show a strong dependence of Ca-II triplet strength on temperature. These lines, together with the (R - I) color index which is known to be a good temperature indicator, were used to estimate the metal abundance and the surface gravity of the present program stars.

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