Characterising anomalous transport in accretion disks from X-ray observations
UNSPECIFIED (2003) Characterising anomalous transport in accretion disks from X-ray observations. In: 3rd Statistical Challenges in Modern Astronomy Conference (SCMA III), PENN STATE UNIV, UNIVERSITY PK, PA, JUL 18-21, 2001. Published in: STATISTICAL CHALLENGES IN ASTRONOMY pp. 423-424.Full text not available from this repository.
We examine the time variation of the total X-ray flux from three sources and find that the signal from the Crab (non-accreting) is uncorrelated, the Cygnus X-1 signal is correlated on timescales up to three years, and in the GRS1915+105 signal correlation may extend to only a few days. The method we use also quantifies the distributions of fluctuations and hence constrains turbulence/instability models of accretion disks.
|Item Type:||Conference Item (UNSPECIFIED)|
|Subjects:||Q Science > QB Astronomy
Q Science > QA Mathematics
|Journal or Publication Title:||STATISTICAL CHALLENGES IN ASTRONOMY|
|Editor:||Feigelson, ED and Babu, GJ|
|Number of Pages:||2|
|Page Range:||pp. 423-424|
|Title of Event:||3rd Statistical Challenges in Modern Astronomy Conference (SCMA III)|
|Location of Event:||PENN STATE UNIV, UNIVERSITY PK, PA|
|Date(s) of Event:||JUL 18-21, 2001|
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