The impacts of GINGA results on QPO models

Details The impacts of GINGA results on QPO models The impacts of GINGA results on QPO models

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..237s&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 237-240 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

1

Frequency Measurement, Ginga Satellite, Periodic Variations, Rotation, Satellite Observation, Stellar Models, Stellar Oscillations, Centroids, Eddington Approximation, Japanese Space Program, Pulsars, Torque, X Ray Binaries

Scientific paper

Quasi-Periodic Oscillation (QPO) observations and the physical causes of QPO are studied. In the light of the recent results from Ginga observations, the physical properties required of QPO models are discussed and the existing QPO models are examined, especially the beat frequency model. The accretion torque theory in the context of the X-ray pulsar QPO is considered.

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