The luminosity function and kinematics of late M dwarf stars.

Details The luminosity function and kinematics of late M dwarf stars. The luminosity function and kinematics of late M dwarf stars.

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..403r&link_type=abstract

The nearby stars and the stellar luminosity function (IAU Colloq. No.76), p. 403 - 409

Computer Science

Luminosity Function:Nearby Stars, M Dwarfs:Nearby Stars, Nearby Stars:Luminosity Function, Nearby Stars:M Dwarfs

Scientific paper

An objective prism survey in the red spectral region was completed in 1976 which covered approximately 2% of the sky at intermediate south galactic latitudes. A kinematically unbiased sample of late red dwarf stars was assembled from the stars detected in this survey. The luminosity function was computed for stars in the range of absolute visual magnitudes from 11.5 to 14.5. The kinematic properties of stars from this sample having absolute magnitudes ≥ 10.5 are compared with those of a group of K and M dwarfs selected from the Catalogue of Stars Within 25 Parsec of the Sun (Woolley et al., 1970).

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