The Determination of the Luminosity Function of Nearby Stars

Details The Determination of the Luminosity Function of Nearby Stars The Determination of the Luminosity Function of Nearby Stars

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..163w&link_type=abstract

In: The Nearby Stars and the Stellar Luminosity Function, Proc. IAU Colloq. 76, Middletown, CT, USA, 13-16 June 1983; A.G. Davis

Physics

134

Scientific paper

The authors present the luminosity function of nearby stars, derived
from Gliese's catalogue, for visual and blue absolute magnitudes. They
discuss some attempts to improve the faint end of the luminosity
function by using Luyten's LHS proper motion catalogue.

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