A model of the source LS I +61 deg 303

Details A model of the source LS I +61 deg 303 A model of the source LS I +61 deg 303

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...289..822l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 289, no. 3, p. 822-826

Mathematics

11

B Stars, Binary Stars, Pulsars, Radio Emission, Stellar Models, Variability, Analysis (Mathematics), Light Curve, Radiant Flux Density, Relativistic Electron Beams, Synchrotron Radiation

Scientific paper

The star LS I +61 deg 303 as radio source with unsual properties is considered. We propose a model of an Induced Pulsator for radio outbursts in LS I +61 deg 303. In our model, the relativistic electrons injected by the radiopulsar are captured by the magnetosphere of the Be-star when the pulsar passed near periastron. Then the captured electrons are cooled slowly due to synchrotron losses. The model was applied to data obtained by Gregory & Taylor in August 1977, August-September 1978 and August-September 1981. These data allow to the determination of parameters of the source LS I +61 deg 303.

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