Mass-Luminosity Relations of Very Low Mass Stars

Details Mass-Luminosity Relations of Very Low Mass Stars Mass-Luminosity Relations of Very Low Mass Stars

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003iaus..211..413s&link_type=abstract

Brown Dwarfs, Proceedings of IAU Symposium #211, held 20-24 May 2002 at University of Hawaii, Honolulu, Hawaii. Edited by Eduard

Physics

Optics

6

Scientific paper

We present new accurate masses at the bottom of the main sequence as
well as an improved empirical mass-luminosity relation for very low mass
stars in the visible and near infrared. Masses were obtained by
combining very accurate radial velocities and adaptive optics images of
multiple stars obtained at different orbital phases.

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