出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：We have presented the Accretion-Ejection Instability (AEI) as an explanation for the Low-
Frequency Quasi-Periodic Oscillation in its most usual form, the C-type. Recently we have shown
that relativistic effects result in another flavor of the AEI, the Relativistic AEI, when the disk gets
close to its last stable orbit. Here we will focus on the consequences on the LFQPO and how this
can be used to explain the less frequent A- and B-type of LFQPO.
