Observations of Alpha Orionis, R Aquilae, and R Aquarii at 14.9 GHz

Details Observations of Alpha Orionis, R Aquilae, and R Aquarii at 14.9 GHz Observations of Alpha Orionis, R Aquilae, and R Aquarii at 14.9 GHz

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..791b&link_type=abstract

Astronomical Journal, vol. 84, June 1979, p. 791-794.

Astronomy and Astrophysics

Astronomy

31

M Stars, Radio Astronomy, Supergiant Stars, Variable Stars, Chromosphere, Continuous Radiation, Ionized Gases, Mira Variables, Stellar Mass Ejection, Stellar Models

Scientific paper

The 14.9-GHz continuum flux densities of the M-type stars Alpha Ori, R Aql, and R Aqr have been measured. For Alpha Ori and R Aql it is suggested that the emission at this frequency is primarily due to ionized gas associated with stellar chromospheres or coronae. For R Aqr a model consistent with available data is proposed in which the variable intensity of the radio emission depends on a variable mass-loss rate for the Mira.

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