Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...392l..31b&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 392, no. 1, June 10, 1992, p. L31-L33.
Astronomy and Astrophysics
Astrophysics
46
Brown Dwarf Stars, Stellar Magnitude, Stellar Temperature, Stellar Color, Stellar Luminosity
Scientific paper
Effective temperatures for the M dwarf stars observed by Berriman and
Reid in 1987 are recalculated, using updated apparent magnitudes where
appropriate. The results show that the corrections to the photometry
have little effect on the derived temperatures, and the Berriman and
Reid results remain a valid temperature scale for low-mass stars.
Berriman Graham
Leggett Sandy K.
Reid Neill
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