A model for A0538-66: The fast flaring pulsar

Details A model for A0538-66: The fast flaring pulsar A model for A0538-66: The fast flaring pulsar

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ans..conf...71m&link_type=abstract

In Max-Planck Inst. Phys. and Astrophys. Accreting Neutron Stars p 71-74 (SEE N83-15179 05-88)

Astronomy and Astrophysics

Astronomy

Pulsars, Solar Flares, X Ray Astronomy, Accretion Disks, Binary Stars, Stellar Mass Accretion

Scientific paper

The conditions for which the onset of the accretion process at
periastron in a highly eccentric binary may take place are discussed.
The optical flare associated with the X-ray flare is interpreted as
reprocessing of X-rays in a envelope surrounding the pulsar.

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