Theoretical stellar chromospheres of late type stars. II - Temperature minima

Details Theoretical stellar chromospheres of late type stars. II - Temperature minima Theoretical stellar chromospheres of late type stars. II - Temperature minima

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....61..515u&link_type=abstract

Astronomy and Astrophysics, vol. 61, no. 4, Nov. 1977, p. 515-521.

Astronomy and Astrophysics

Astrophysics

24

Chromosphere, Late Stars, Stellar Atmospheres, Stellar Temperature, Semiempirical Equations, Shock Heating, Stellar Models

Scientific paper

The theory of heating by short period acoustic waves is applied to predict the height of shock formation and the acoustic flux at the base of the chromosphere for stars with effective temperatures of 4000 to 6500 K and log g of 2 to 4. These predictions are compared with heights of temperature minima and with chromospheric radiation losses computed from semiempirical models.

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