Radio Emission of YZ CMi at 1.6, 2 and 3.6 CM

Details Radio Emission of YZ CMi at 1.6, 2 and 3.6 CM Radio Emission of YZ CMi at 1.6, 2 and 3.6 CM

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aca....44...75r&link_type=abstract

Acta Astronomica, v.44, pp.75-79, (1994).

Astronomy and Astrophysics

Astronomy

Stars: Activity, Stars: Late Type, Stars: Individual: Yz Cmi

Scientific paper

Observations at two epochs at the currently shortest wavelengths accessible with the VLA system are presented. YZ CMi was observed to be surprisingly radio bright at these wavelengths which, taken together with previous 6 -- 20cm observations and variability between the epochs, suggests non-thermal origin of electrons producing the gyrosynchrotron emission.

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