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Radiation-driven acceleration in the expanding WR140 dust shell
The Wolf–Rayet (WR) binary system WR140 is a close (0.9–16.7 mas; ref. (1)) binary star consisting of an O5 primary and WC7 companion(2) and is known as the archetype of episodic dust-producing WRs. Dust in WR binaries is known to form in a confined stream originating from the collision of the two s...
| Autores principales: | , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2022
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9556302/ https://www.ncbi.nlm.nih.gov/pubmed/36224416 http://dx.doi.org/10.1038/s41586-022-05155-5 |