Optical Precursors to Black Hole X-ray Binary Outbursts: An evolving synchrotron jet spectrum in Swift J1357.2-0933
We present six years of optical monitoring of the black hole candidate X-ray binary Swift J1357.2-0933, during and since its discovery outburst in 2011. On these long timescales, the quiescent light curve is dominated by high amplitude, short term (seconds-days) variability spanning ~ 2 magnitudes,...
| Main Authors: | , , , , , , |
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| Format: | Journal Article |
| Published: |
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2018
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| Online Access: | http://hdl.handle.net/20.500.11937/57926 |