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[vsnet-alert 5827] Re: New Haseda variable (HadV82) = WR104



Re: New Haseda variable (HadV82) = WR104

   Since the rotation period of the spiral (Tuthill et al. 1999, Nature
398, 487: "A dusty pinwheel nebula around the massive star WR 104") is
reported to be 220 d, observations at higher frequencies are encouraged.

Regards,
VSNET Collaboration team

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