Dear John, Dear colleagues, I also think, that both indications (B-R from USNO A2.0 and the apparently slow variation, deduced from about 10 observations in different nights within 1-2 months), which I take for classification as a "SR"-variable are not unambigous. If a "SR"-variable would be in fact a short period variable, there could arise wrong B-R values, even if the epochs of the plates differ only few days. So I always mention in the VSNET-postings, that the colour and the apparently slow change in brightness "suggest" a SR-variable. But I see, especially because of the X-ray source BrhV84 (a "SR-variable" transformed in a likely short period variable) that I have to write instead of "Other types of l o n g period variability cannot be excluded" in future "Other types of variability cannot be excluded" in my VSNET-postings. Best wishes, Klaus Bernhard > > The epochs of the USNO A2.0 plates that this variable appears upon are > dated 1979 for the blue one and 1984 for the red one. > > Using magnitudes from two totally different epochs for an avowedly variable > object in an attempt to decide a colour index and subsequently a > variability class is a somewhat problematic exercise. > > John