Photometric variability of WC9 stars

Monthly Notices of the Royal Astronomical Society(2009)

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摘要
Do some Wolf–Rayet stars owe their strong winds to something else besides radiation pressure? The answer to this question is still not entirely obvious, especially in certain Wolf–Rayet subclasses, mainly WN8 and WC9. Both of these types of Wolf–Rayet stars are thought to be highly variable, as suggested by observations, possibly due to pulsations. However, only the WN8 stars have so far been vigo...
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stars: carbon,circumstellar matter,stars: individual: WR76,stars: variables: other,stars: Wolf–Rayet
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