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Understanding structure in line-driven stellar winds using ultraviolet spectropolarimetry in the time domain.
- Published in:
- Astrophysics & Space Science, 2022, v. 367, n. 12, p. 1, doi. 10.1007/s10509-022-04142-6
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- Article
Ultraviolet spectropolarimetry: conservative and nonconservative mass transfer in OB interacting binaries.
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- Astrophysics & Space Science, 2022, v. 367, n. 12, p. 1, doi. 10.1007/s10509-022-04106-w
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- Article
UV spectropolarimetry with Polstar: massive star binary colliding winds.
- Published in:
- Astrophysics & Space Science, 2022, v. 367, n. 12, p. 1, doi. 10.1007/s10509-022-04102-0
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- Article
The origin and impact of Wolf-Rayet-type mass loss.
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- Proceedings of the International Astronomical Union, 2022, v. 16, n. S366, p. 21, doi. 10.1017/S1743921322000400
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- Article
Spectroscopy of complete populations of Wolf-Rayet binaries in the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2018, n. S346, p. 307, doi. 10.1017/S1743921319001303
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- Article
Massive stars in advanced evolutionary stages, and the progenitor of GW150914.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S329, p. 223, doi. 10.1017/S1743921317002563
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- Article
WR 148 and the not so compact companion.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S329, p. 427, doi. 10.1017/S174392131700357X
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- Article
The formation of Wolf-Rayet stars in the SMC is not dominated by mass transfer.
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- Proceedings of the International Astronomical Union, 2016, v. 12, n. S329, p. 445, doi. 10.1017/S1743921317001995
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- Article