Radio Emission from Flare Star V371 Orionis

Details Radio Emission from Flare Star V371 Orionis Radio Emission from Flare Star V371 Orionis

Sep 1963

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1963natur.199..991s&link_type=abstract

Nature, Volume 199, Issue 4897, pp. 991-993 (1963).

Physics

18

Scientific paper

DURING the past three years the Division of Radio-physics, Commonwealth Scientific and Industrial Research Organization, Sydney, Australia, has made a systematic attempt to detect radio emission from a number of the so-called flare stars situated in the Sun's vicinity. Slee, Patston and Higgins1 have described the earlier work and results. Lovell, Whipple and Solomon2 have also recently published the results of a similar flare-star survey conducted at Jodrell Bank. Taken together, these two surveys have established with a reasonable degree of certainty that at least some of the flares on the six red dwarfs examined were accompanied by detectable radio emission.

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