Estimation of Stellar Astrophysical Parameters with the Gaia Baseline Photometric System

Details Estimation of Stellar Astrophysical Parameters with the Gaia Baseline Photometric System Estimation of Stellar Astrophysical Parameters with the Gaia Baseline Photometric System

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..401m&link_type=abstract

Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology ASP Conference Series, Vol. 353, Proceedings of the Confe

Physics

Scientific paper

One classification scheme in the minimum distance method is applied to
the most recent Gaia simulated photometric data, the achieved
classification accuracies are given for some normal and low metallicity
stars.

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