Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....82..249b&link_type=abstract
Astronomy and Astrophysics, vol. 82, no. 1-2, Feb. 1980, p. 249-252.
Astronomy and Astrophysics
Astronomy
142
Atmospheric Models, Diameters, Infrared Astronomy, Stellar Atmospheres, Stellar Temperature, Temperature Scales, Infrared Radiation, Radiant Flux Density, Stellar Luminosity, Stellar Spectra
Scientific paper
An alternative method of using the infra-red flux method for determining stellar effective temperatures and angular diameters is presented. Tables are presented giving the ratios of integrated stellar fluxes to monochromatic fluxes as a function of wavelength, gravity and effective temperature for two model atmospheres. Measured values of these ratios for 28 stars are used in conjunction with these tables to determine values of Te and θ for them. The results have been applied to the construction of a stellar temperature scale for luminosity class V stars.
Blackwell D. E.
Petford A. D.
Shallis M. J.
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