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- W19730654 abstract "WR147 was first discovered to be a strong radio, X-ray and infra-red emission source by Caillault et al. (1985). It was classified as a WN8 type star with a very large mass loss rate and unusual radio emission (α < 0) for a thermal source. This unusual behaviour was explained by MERLIN (Moran et al. 1989) and VLA (Churchwell et al. 1992) observations in which it was resolved into two components: a ‘thermal’ source associated with the Wolf-Rayet star and a non-thermal component ∼ 600 mas to the north. Churchwell et al. showed that the southern component had the expected spectral index of α ≃ 0.6 for free-free emission from a stellar wind. They also showed that the northern component had a spectral index of α ≃ −0.5 and was therefore a non-thermal source, now thought to be due to a colliding wind region." @default.
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- W19730654 date "1999-01-01" @default.
- W19730654 modified "2023-10-14" @default.
- W19730654 title "MERLIN observations of WR 147 (WN8(h)+B0.5V)" @default.
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- W19730654 doi "https://doi.org/10.1017/s0074180900205913" @default.
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