Long-term X-ray variation of the colliding wind Wolf-Rayet binary WR 125

27 Dec 2018 Midooka Takuya Sugawara Yasuharu Ebisawa Ken

WR 125 is considered as a Colliding Wind Wolf-rayet Binary (CWWB), from which the most recent infrared flux increase was reported between 1990 and 1993. We observed the object four times from November 2016 to May 2017 with Swift and XMM-Newton, and carried out a precise X-ray spectral study for the first time... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA