Accretion-Ejection Instability, LFQPO and lag structure of microquasars

Details Accretion-Ejection Instability, LFQPO and lag structure of microquasars Accretion-Ejection Instability, LFQPO and lag structure of microquasars

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..797..213v&link_type=abstract

INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP Conference Proceedings, Volume 797, pp. 213-218 (2005).

Computer Science

X-Ray Binary Stars, Quasars, Accretion, X-Ray Binaries, Quasars, X-Ray

Scientific paper

The Accretion-Ejection Instability (AEI) has been proposed to explain the low frequency Quasi-Periodic Oscillation (QPO) observed in low-mass X-Ray Binaries. Its frequency, typically a fraction of the Keplerian frequency at the disk inner radius, is in the right range indicated by observations. I will briefly review the basic of the instability. In a second part I will focus on a simple model to explain the complex lag structure between the hard and soft X-ray observed in microquasars such as GRS 1915+105.

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