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X-ray study of WR 48-6: A possible colliding wind binary: X-ray study of WR 48-6: a possible colliding...
DOI: 10.1007/s12036-025-10039-x Bibcode: 2025JApA...46...16J

Tej, Anandmayee; Pandey, Jeewan C.; Jadoliya, Vishal

This paper presents an investigation of the X-ray emission associated with the Wolf–Rayet star, WR 48-6, using observations from the XMM-Newton and Chandra X-ray telescopes covering two epochs separated by eleven months. The X-ray spectrum of WR 48-6 is well explained by a two-temperature plasma model, with cool and hot plasma temperatures of

2025 Journal of Astrophysics and Astronomy
XMM-Newton 0