An additional soft X-ray component in the dim low/hard state of black hole binaries
An additional soft X-ray component in the dim low/hard state of black hole binaries
We test the truncated disc models using multiwavelength (optical/UV/X-ray) data from the 2005 hard state outburst of the black hole SWIFT J1753.5-0127. This system is both fairly bright and has fairly low interstellar absorption, so gives one of the best datasets to study the weak, cool disc emission in this …