Barnard's Star and the dM Effective Temperature Scale

Details Barnard's Star and the dM Effective Temperature Scale Barnard's Star and the dM Effective Temperature Scale

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...202.3205d&link_type=abstract

American Astronomical Society Meeting 202, #32.05; Bulletin of the American Astronomical Society, Vol. 35, p.743

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Scientific paper

The recently measured angular diameter of Barnard's Star, together with its large and precise parallax, and a spectral energy distribution that extends from the ultraviolet to almost 12 μ m establish some of the star's fundamental properties: its bolometric luminosity, radius, and effective temperature. Accurate knowledge of these parameters leads in turn to useful constraints on its metallicity and mass. Effective temperature estimates obtained by other, less direct methods are compared with the definitive result.

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