Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

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 12.

Visualization of the WR 112 models simulated at the epoch of the near-IR AO observations. Top row: dust column density models. Bottom row: O-star wind column density models. Left column: accelerating model of WR 112 as viewed from Earth. Middle column: face-on view of the accelerating model (setting the observer at the left of the frame looking right). Right column: face-on models simulated without acceleration to visualize its effects by comparison with the middle column (observer at the left of the frame looking right).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse