On the observation of stellar temperature minima

Details On the observation of stellar temperature minima On the observation of stellar temperature minima

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....59..177s&link_type=abstract

Astronomy and Astrophysics, vol. 59, no. 2, July 1977, p. 177-179.

Astronomy and Astrophysics

Astrophysics

3

Brightness Temperature, Chromosphere, Stellar Atmospheres, Stellar Temperature, Extremum Values, Infrared Spectra, Prediction Analysis Techniques, Radio Spectra, Temperature Measurement, Ultraviolet Spectra, Wavelengths

Scientific paper

Minima of brightness temperature due to the presence of stellar temperature minima are predicted in the UV, infrared, and radio-frequency ranges. The theoretical temperature minima for stars in the range of effective temperature from 4000 to 6500 K and log g from 2 to 4 used in this work are calculated on basis of the short-period acoustic heating theory.

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