Effective temperatures of late-type stars - The field giants from K0 to M6

Details Effective temperatures of late-type stars - The field giants from K0 to M6 Effective temperatures of late-type stars - The field giants from K0 to M6

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235..126r&link_type=abstract

Astrophysical Journal, Part 1, vol. 235, Jan. 1, 1980, p. 126-137.

Astronomy and Astrophysics

Astronomy

421

Giant Stars, Late Stars, Stellar Atmospheres, Stellar Spectra, Stellar Temperature, Bolometers, Diameters, Infrared Astronomy, Infrared Photometry, Lunar Occultation, M Stars, Stellar Models, Stellar Spectrophotometry

Scientific paper

Angular diameters from lunar occultation are combined with infrared photometry to determine effective temperatures for K0-M6 giants. The relations between effective temperature and color temperature, MK spectral type, V-K color, and I(104)-L color are derived. The principal result is a general increase in effective temperature for the cooler spectral types compared to previous calibrations. Throughout the temperature range studied, excellent agreement is obtained with recent model atmosphere computations.

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