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The semi-regular variable V CVn is having a bit of a moment from a polarisation point of view. It’s polarisation is inversely correlated with brightness and just recently has jumped to around 5.8 %, approaching levels that were last seen in the 1990’s (HPOL). If anyone is able and willing to add it to their photometric observations list for the next 2-3 weeks – nightly BVRI would be wonderful – that would be much appreciated. As luck would have it I’m away from home and kit until the 20th September. Many thanks.
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