Accretion-EJection Instability: new results on QPOs

Details Accretion-EJection Instability: new results on QPOs Accretion-EJection Instability: new results on QPOs

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003head....7.1721v&link_type=abstract

American Astronomical Society, HEAD meeting #7, #17.21; Bulletin of the American Astronomical Society, Vol. 35, p.628

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The Accretion-Ejection Instability has been proposed has been proposed to explain the low frequency Quasi-Periodic Oscillation (QPO) observed in low-mass X-Ray Binaries, in particular Black-Hole candidates. Its frequency, typically a fraction of the Keplerian frequency at the disk inner radius, is exactly in the range indicated by observations. We will show how this instability is able to produce a modulation of the X-ray flux and what are the characteristic of this modulation.

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