Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...396..173t&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 396, no. 1, Sept. 1, 1992, p. 173-177.
Astronomy and Astrophysics
Astrophysics
32
Brown Dwarf Stars, Faint Objects, Mass To Light Ratios, Stellar Luminosity, Stellar Mass, Infrared Photometry, Main Sequence Stars, Near Infrared Radiation
Scientific paper
A determination of the luminosity and mass functions is given for field stars at the bottom of the main sequence as the first results from a 320 sq deg survey based on both optical and near-infrared photometry. The luminosity and mass functions are determined with an order of magnitude higher precision than previous studies achieve. No evidence is found for a mass function steepening toward the H-burning limit.
Mould Jeremy R.
Reid Iain Neill
Tinney Chris G.
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