Results from the Nearby Stars (NStars) Program

Details Results from the Nearby Stars (NStars) Program Results from the Nearby Stars (NStars) Program

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21934502c&link_type=abstract

American Astronomical Society, AAS Meeting #219, #345.02

Astronomy and Astrophysics

Astronomy

Scientific paper

Progress is continuing toward a final omnibus publication containing new precise spectral types, basic physical parameters, and (where relevant) measures of the chromospheric activity for the 3600 stars earlier than M0 within 40 parsecs of the Sun. In this poster we review recent improvements in the derivation of the basic physical parameters (Teff, log(g), [M/H], and microturbulent velocity) via fits to model fluxes and spectra, and in the transformation of our measures of chromospheric activity to the Mount Wilson system.

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