FORCASTing the Spectroscopic Dust Properties of the WC+O Binary WR 137 with SOFIA
WR 137 (HD 192641) is a binary system consisting of a carbon-rich Wolf–Rayet (W-R) star and an Oe companion star in a 13 yr orbit. Near periastron, the winds of the two stars collide and form carbonaceous dust. We obtained three mid-infrared grism spectra of the system with SOFIA and FORCAST during...
Main Authors: | Megan J. Peatt, Noel D. Richardson, Peredur M. Williams, Nicole Karnath, Victor I. Shenavrin, Ryan M. Lau, Anthony F. J. Moffat, Gerd Weigelt |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acf201 |
Similar Items
-
Constraints on the Binarity of the WN3/O3 Class of Wolf–Rayet Stars
by: Philip Massey, et al.
Published: (2023-01-01) -
Testing He ii Emission from Wolf–Rayet Stars as a Dust Attenuation Measure in Eight Nearby Star-forming Galaxies
by: Daniel Maschmann, et al.
Published: (2024-01-01) -
Newly Discovered Wolf–Rayet Stars in M31
by: Kathryn F. Neugent, et al.
Published: (2023-01-01) -
UV Spectroscopy of Massive Stars
by: D. John Hillier
Published: (2020-08-01) -
The Wolf–Rayet Content of the Galaxies of the Local Group and Beyond
by: Kathryn Neugent, et al.
Published: (2019-08-01)