Colliding winds in five WR+O systems of the Southern hemisphere
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/424/3/1601/2975926/424-3-1601.pdf
Reference42 articles.
1. Magellanic Cloud WC/WO Wolf-Rayet stars - II. Colliding winds in binaries
2. Exact, Algebraic Solutions of the Thin-Shell Two-Wind Interaction Problem
3. WR 110: A SINGLE WOLF-RAYET STAR WITH COROTATING INTERACTION REGIONS IN ITS WIND?
4. Spectroscopic Studies of O-Type Stars. I. Classification and Absolute Magnitudes
5. The Quadruple Wolf‐Rayet System GP Cephei: Spectral Types, Masses, Mass‐Loss Rate, and Colliding Winds
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1. Using a new spectral disentangling approach to ascertain whether the massive binary HDE 228766 contains a Wolf–Rayet star;Monthly Notices of the Royal Astronomical Society;2024-07-05
2. Colliding winds in WR21 and WR31 – I. The X-ray view;Monthly Notices of the Royal Astronomical Society;2023-09-06
3. The Arches cluster revisited – IV. Observational constraints on the binary properties of very massive stars;Monthly Notices of the Royal Astronomical Society;2023-02-10
4. Modeling the Optical to Ultraviolet Polarimetric Variability from Thomson Scattering in Colliding-wind Binaries;The Astrophysical Journal;2022-06-28
5. New X-ray detections of known Wolf–Rayet stars;Monthly Notices of the Royal Astronomical Society;2020-12-10
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