Some remarks on the quasiperiodic variation mechanisms at accreting magnetized objects

Details Some remarks on the quasiperiodic variation mechanisms at accreting magnetized objects Some remarks on the quasiperiodic variation mechanisms at accreting magnetized objects

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..203l&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Jan.-Feb. 1987, p. 203, 204. In Russian.

Astronomy and Astrophysics

Astronomy

Neutron Stars, Periodic Variations, Radiant Flux Density, Stellar Magnetic Fields, Stellar Mass Accretion, White Dwarf Stars, Axes Of Rotation, Stellar Orbits

Scientific paper

A hydrodynamic instability in the polar cap of an accreting neutron star
or a white dwarf is considered as a possible cause of quasiperiodic
light variations. Simple relationships are derived which exist between
observable parameters of accreting stars and bursts.

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