Atmospheric Thermal Structure of a Sample of M Type Giants

Details Atmospheric Thermal Structure of a Sample of M Type Giants Atmospheric Thermal Structure of a Sample of M Type Giants

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.282..743j&link_type=abstract

Astrophysics and Space Science, v. 282, Issue 4, p. 743-747 (2002).

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

Vibrational temperatures in the atmospheres of nine M type giants of luminosity class III and subtypes M2-M8 located in the Galactic plane have been determined from the γ band system of the TiO molecule. The relationship between Texc and Teff has been established in agreement with the chosen Teff calibration scale. The deviation of Texc with recspect to Teff for our stars has been used as an indicator of the depth of the atmospheric layers in which the molecular bands are formed.

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