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Revealing the Accelerating Wind in the Inner Region of Colliding-wind Binary WR 112

  • Authors: John D. Monnier, Yinuo Han, Michael F. Corcoran, Sanne Bloot, Joseph R. Callingham, William Danchi, Philip G. Edwards, Lincoln Greenhill, Kenji Hamaguchi, Matthew J. Hankins, Ryan Lau, Jon M. Miller, Anthony F. J. Moffat, Garreth Ruane, Christopher M. P. Russell, Anthony Soulain, Samaporn Tinyanont, Peter Tuthill, Jason J. Wang, Peredur M. Williams

John D. Monnier et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 2.

Left: false-color broadband (0.2–10 keV) Chandra image of the WR 112 field from ObsID 25129. Center: Chandra image, ObsID 29739. Right: 2MASS J-band (λ ∼ 1.23 μm) image of WR 112. Contours from the 2MASS image are overlaid on the Chandra images. Note that, aside from WR 112, there are no other J-band sources clearly detected in the Chandra X-ray images.

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