Periodicities in the radio emission of UX Arietis?

Details Periodicities in the radio emission of UX Arietis? Periodicities in the radio emission of UX Arietis?

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...278l..51n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 278, no. 2, p. L51-L53

Astronomy and Astrophysics

Astronomy

13

Binary Stars, Circular Polarization, Flare Stars, Radio Astronomy, Radio Emission, Energy Distribution, K Stars, Radio Telescopes, Synchrotron Radiation

Scientific paper

Observations of UX Arietis, in the range 9 mm - 21 cm, have been performed with the Effelsberg 100-m radio-telescope from December 1992 to May 1993. The data seem to indicate that the most powerful events take place in coincidence with the orbital phase, in which the cooler K-star is in front. Also some regular variation in the circular polarization seem to be present in the data. These results however, although very interesting, deserve to be confirmed by further, more regular observations.

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