Radio emission and chromosphere of Betelgeuse

Details Radio emission and chromosphere of Betelgeuse Radio emission and chromosphere of Betelgeuse

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....96..102w&link_type=abstract

Astronomy and Astrophysics, vol. 96, no. 1-2, Mar. 1981, p. 102-105.

Astronomy and Astrophysics

Astrophysics

14

Chromosphere, Radio Emission, Red Giant Stars, Semiregular Variable Stars, Stellar Radiation, Supergiant Stars, Atmospheric Density, Atmospheric Models, Atmospheric Temperature, Brightness, Radio Spectra

Scientific paper

The implications of the recently established two component radio
emission of Betelgeuse for its atmospheric structure are studied. It is
shown that the star must have an extended chromosphere with a
temperature of about 8600 K. An attempt is made to incorporate this fact
consistently into the radial variation of temperature and density.

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