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- W1520346811 abstract "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." @default.
- W1520346811 created "2016-06-24" @default.
- W1520346811 creator A5083891857 @default.
- W1520346811 date "2005-01-01" @default.
- W1520346811 modified "2023-10-14" @default.
- W1520346811 title "Accretion-Ejection Instability, LFQPO and lag structure of microquasars" @default.
- W1520346811 doi "https://doi.org/10.1063/1.2130235" @default.
- W1520346811 hasPublicationYear "2005" @default.
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