Speaker
Maxime Parra
(Ehime University)
Description
Despite having one of the most detailed outburst coverage among BHLMXBs, the long term behavior of the wind in 4U 1630-47 remains poorly known. We thus performed an exhaustive study of archival X-ray observations of the source, combining Chandra, NICER, NuSTAR, Suzaku and XMM-Newton, for more than 200 epochs spanned over 9 separate outbursts and two decades, complemented by Swift-BAT and INTEGRAL. I will present our results for the long term evolution of the lines and wind, including new diagnostics made possible by the high energy coverage.
Primary author
Maxime Parra
(Ehime University)
