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[vsnet-newvar 1699] HD 932 is NOT a Cepheid variable, NOR of 10.3 day period




ENTIRELY CONTRARY to an earlier post I made :-

HD 932 has turned out to be a variable of probably less than a day's
period, and it may not even be a pulsator (eg, RRc), but an EW star
instead.  A5 spectral type is still a bit early for the latter, and RRc
type is ideal for that, so matters are still not certain.


John Greaves


(PS  I'm gobsmacked!)

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