5 GHz Emission from ß Persei

Details 5 GHz Emission from ß Persei 5 GHz Emission from ß Persei

Aug 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973natur.244..270p&link_type=abstract

Nature, Volume 244, Issue 5414, pp. 270-272 (1973).

Computer Science

7

Scientific paper

THE triple star system β Persei (Algol) is an erratic radio source1 which has occasional periods of activity lasting for several days. Jones and Woolf2 suggest that the emission results from mass transfer between Algol A and B, the components of the 2.8 d eclipsing binary. Hjellming3 has discussed the parameters of possible models for the emission region.

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