New Limits on the Surface Density of M Dwarfs from CCD and Photographic Data

Details New Limits on the Surface Density of M Dwarfs from CCD and Photographic Data New Limits on the Surface Density of M Dwarfs from CCD and Photographic Data

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf...85b&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Physics

1

Scientific paper

The authors report on a search of the FOCAS (Faint Object Classification and Analysis System) catalog of stars and galaxies to 24th J photographic magnitude and a preliminary search of CCD data to 26th magnitude for extreme M dwarfs. This program extends earlier searches to 100 pc (photographic) and 400 pc (CCD) at high latitude for Mv = 19 mag, thus sampling whatever halo or fat disk population of extreme M dwarfs and brown dwarfs may be there.

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