Detailed analysis of cool giants with low microturbulent velocity

Details Detailed analysis of cool giants with low microturbulent velocity Detailed analysis of cool giants with low microturbulent velocity

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....93..315f&link_type=abstract

Astronomy and Astrophysics, vol. 93, no. 1-2, Jan. 1981, p. 315-319.

Astronomy and Astrophysics

Astrophysics

4

Abundance, Atmospheric Models, Atmospheric Turbulence, G Stars, Giant Stars, Stellar Atmospheres, Barium, Data Reduction, Infrared Spectrophotometers, Iron, K Stars, Stellar Gravitation, Stellar Spectrophotometry

Scientific paper

Five G-K giants have been analyzed by using the curve-of-growth method
and model atmospheres. The significance of the low microturbulent
velocities found for four of the five giants and the trend toward an
overabundance of barium in these giants are discussed.

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