A search for slowly varying radio continuum emission from UV Ceti stars

Details A search for slowly varying radio continuum emission from UV Ceti stars A search for slowly varying radio continuum emission from UV Ceti stars

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...205..472s&link_type=abstract

Astrophysical Journal, vol. 205, Apr. 15, 1976, pt. 1, p. 472-474.

Astronomy and Astrophysics

Astronomy

2

Brightness Temperature, Late Stars, M Stars, Radio Emission, Variable Stars, Continuous Radiation, Radiant Flux Density, Radio Astronomy, Stellar Luminosity

Scientific paper

The paper presents results of a search conducted at the Arecibo Observatory for variable 430-MHz emission from the active flare stars EQ Peg, YZ CMi, and AD Leo. No statistically significant evidence for slowly varying emission is found to a level of 0.05 Jy for AD Leo, 0.018-0.021 Jy for YZ CMi, and 0.009-0.018 Jy for EQ Peg. Upper limits of about 10 trillion K are determined for the brightness temperature of active radio regions on these stars at the time of the observations.

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