Luminosities and temperatures of M dwarf stars from infrared photometry

Details Luminosities and temperatures of M dwarf stars from infrared photometry Luminosities and temperatures of M dwarf stars from infrared photometry

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974aj.....79.1056v&link_type=abstract

Astronomical Journal, vol. 79, Oct. 1974, p. 1056-1072.

Astronomy and Astrophysics

Astronomy

208

Dwarf Stars, Infrared Photometry, M Stars, Stellar Luminosity, Stellar Spectrophotometry, Stellar Temperature, Bolometers, Emission Spectra, Hertzsprung-Russell Diagram, Infrared Spectra, Late Stars, Main Sequence Stars, Tables (Data), Temperature Measurement

Scientific paper

Bolometric magnitudes for a large number of M type dwarf stars, obtained by broadband infrared photometry at 1.65, 2.2, and 3.5 microns, are reviewed. The data obtained indicate that one parameter is sufficient to describe the blanketing in all of the UBVRI bands for all types of M dwarfs. In general, late M dwarfs seem to have lower effective temperatures than are predicted by theoretical models.

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