@inproceedings{48c231c1a57f4bed9c63f5a723dc951f,
title = "The X-ray Binary analogy to the first AGN QPO",
abstract = "We examine the different QPOs seen in X-ray Binaries for an analogous signal to the first AGN QPO. Simple mass scaling rules out the low-frequency and standard high-frequency QPOs. However, the rather unique 67 Hz QPO of GRS1915+105 scales to imply the source is accreting at around Eddington as supported by the SED. The 67 Hz QPO is seen when GRS1915+105 is in a very similar spectral state to that of REJ1034+396 and the power spectrum continuum slopes below the QPOs, are consistent. The difference in normalisation is suggested to be intrinsic and subsequent bandpass corrections yield consistent values.",
keywords = "AGN, Black holes, QPO, Seyferts",
author = "M. Middleton and C. Done and M. Gierli{\'n}ski",
year = "2010",
month = jul,
day = "15",
doi = "10.1063/1.3475248",
language = "English",
isbn = "9780735407954",
volume = "1248",
series = "AIP Conference Proceedings",
publisher = "AIP Publishing",
pages = "325--328",
editor = "A. Comastri and L. Angelini and M. Cappi",
booktitle = "X-ray Astronomy-2009",
address = "United States",
note = "International Conference on X-ray Astronomy-2009: Present Status, Multi-Wavelength Approach and Future Perspectives ; Conference date: 07-09-2009 Through 11-09-2009",
}