An Orbit for a Massive Wolf–Rayet Binary in the LMC: An Example of Binary Evolution
Wolf–Rayet (WR) stars are helium-burning, evolved massive stars which have had most of their hydrogen-rich outer layers removed, either through stellar winds and/or binary stripping. Here, we report on LMC 173-1, a WN3+O binary located in the Large Magellanic Cloud (LMC). Using spectra obtained from...
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| Asıl Yazarlar: | , , , , , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2026-01-01
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| Seri Bilgileri: | The Astrophysical Journal |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/1538-4357/ae5187 |
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