Nested dust shells around the Wolf–Rayet binary WR 140 observed with JWST
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-022-01812-x.pdf
Reference43 articles.
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2. Lau, R. M. et al. Revisiting the impact of dust production from carbon-rich Wolf-Rayet binaries. Astrophys. J. 898, 74 (2020).
3. Endo, I. et al. Detection of a Broad 8 μm UIR feature in the mid-infrared spectrum of WR 125 observed with Subaru/COMICS. Astrophys. J. 930, 116 (2022).
4. Crowther, P. A. Physical properties of Wolf-Rayet stars. Annu. Rev. Astron. Astrophys. 45, 177–219 (2007).
5. Usov, V. V. Stellar wind collision and dust formation in long-period, heavily interacting Wolf-Rayet binaries. Mon. Not. R. Astron. Soc. 252, 49–52 (1991).
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