The star LSI +61 degrees 303 as a radio source with unusual properties
is considered. We propose a model of an Induced Pulsator for radio ou
tbursts in LSI +61 degrees 303. In our model, the relativistic electro
ns injected by the radiopulsar are captured by the magnetosphere of th
e Be-star when the pulsar passed near periastron. Then the captured el
ectrons are cooled slowly due to synchrotron losses. The model was app
lied to data obtained by Gregory and Taylor in August 1977, August-Sep
tember 1978 and August-September 1981. These data allow to the determi
nation of parameters of the source LSI +61 degrees 303.