No CrossRef data available.
Article contents
X-ray variability of accreting black hole systems: propagating-fluctuation scenario
Published online by Cambridge University Press: 01 August 2006
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Propagating fluctuation models can reproduce fundamental properties of the variability observed in the X-ray light curves of accreting black hole systems. We explore this type of model and show how extended emitting regions introduce at the same time energy dependent power spectral densities (PSD) and time lags between different energy bands.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S238: Black Holes from Stars to Galaxies – Across the Range of Masses , August 2006 , pp. 319 - 320
- Copyright
- Copyright © International Astronomical Union 2007
References
Arévalo, P., Papadakis, I., Uttley, P., McHardy, I. & Brinkmann, W. 2006, MNRAS 372, 401CrossRefGoogle Scholar
You have
Access