出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：We give a short overview the Accretion-Ejection Instability and show how it provides a good
model to explain the Low-Frequency QPO’s from microquasars. From that we show how the
Magnetic Flood Scenario can explain the variability class b of GRS 1915+105 and how to extend
it beyond that class.
