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    stars of the moment

    From: Joe Patterson <jop_at_astro.columbia.edu>
    Date: Mon, 8 Feb 1999 11:48:00 -0500 (EST)
    Dear CBAers,
    
    Re starry targets, there are big developments to report.  For
    northerners, the very very scattered coverage so far indicates that
    BK Lyn (= Cnc 1 = PG0917+342) has probably jumped to a new period
    and greatly increased its amplitude.  Thus it's now the best target
    for all northern scopes.  My guess at this early date is that it's
    imitating the act V603 Aql performed in 1994.  But we can much more
    satisfactorily study this phenomenon now, because our tools are better
    now, and because there's a big difference between February nights and
    July nights!
    
    The best comparison star appears to be the star 2' ESE from the variable,
    near the little background galaxy.  This star has V=13.22, B-V=0.94
    according to Henden & Honeycutt.  Not our favorite color, but the best
    overall choice I think.  You should get Var-Comp values around +1.7
    in unfiltered light with a red-sensitive chip (like practically all 
    CCDs).           
    
    Another star that we're studying closely is DW UMa, which dived into a
    low state a few weeks ago.  Nice target for the biggest scopes, which
    can perhaps resolve the time scales around the eclipse (18th-20th mag).
    
    For southerners, our old friend Men 1 = AH Men has just thrown us a
    curve ball (Kiwis please translate to the cricket equivalent).  For 4
    years it always tossed at us a complex spectrum of periods near 3
    hrs: at 2.95, 3.05, and 3.30 hrs.  Usually two were simultaneously
    present, accompanied by complex harmonics.  During December 1998, we got 
    extensive coverage from Piet Meintjes in South Africa and Marc Bos in
    New Zealand, and some from Jonathan Kemp in Chile.  Can't argue with
    that longitude coverage.  Great was my chagrin when a first pass at 
    the data showed *no* convincing periodic signals near 3 hours!  Some 
    of the familiar harmonics were weakly present, and Piet may be able to
    dig out our old friends after a close look, but the overall outlook was
    disappointing.
    
    The moral I suppose is that even the "permanent" superhumpers need to rest
    every so often.  Fair enough; I just wish they wouldn't rest during a 
    multi-longitude campaign.  And the other moral is that we should avoid 
    this star for a coupla years.  Let's get friendly instead with the other 
    bright short-period CV in the southern summer sky - RR Pic - and also
    start the year up on SW Sex (note the coords of this star in DWS are
    incorrect in the RA listing, but correct in the alphabetical listing; 
    there's a chart and a comp and good coords in ye olde CBA website).
    
    Finally I'd be interested in hearing your plans for attendance at the
    PASP meeting in Toronto, which several of us will attend and even have
    a little CBA table.  Personally I also plan to attend the previous week's
    photometry conference in New Zealand, where we have accumulated such a 
    strong network despite my never having met any of the people involved.
    
    We just revised the website a bit - with BK Lyn flashing to remind you!
    
    
    
              Joe
    
    Received on 8 Feb 1999