Accretion disk parameters in HLX-1
We estimate the outer radius of the accretion disk in HLX-1 from its optical brightness and from the exponential timescale of the decline in the X-ray lightcurve after an outburst. We find that the disk is an order of magnitude smaller than the semimajor axis of the orbit. If the disk size is determ...
| Main Authors: | , |
|---|---|
| Format: | Conference Paper |
| Published: |
2012
|
| Online Access: | http://hdl.handle.net/20.500.11937/15678 |