June 1992 • 1992ApJ...392L..31B
Authors • Berriman, Graham • Reid, Neill • Leggett, S. K.
Abstract • 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.
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