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    stars for october

    From: Joe Patterson <jop_at_astro.columbia.edu>
    Date: Thu, 29 Sep 2005 23:42:32 -0400 (EDT)
    Dear CBAers,
    
    The LS Peg campaign is ready for wrap-up now.  The star displayed a
    handsome negative superhump throughout, with coverage dense enough to
    enable sensitive search for some of the lesser-known effects (especially
    the precession period itself).  It's not going to get any better, so it's
    time to quit.
    
    Two other prime targets du jour are Cep 1 and HS2339+30 ("And"). These are
    not eliciting much attention!  I realize they're tough - around 16.5 - but
    the Moon's outa the way and these stars, likely to be among the oldest of
    cataclysmic binaries, will repay handsomely in terms of the science reaped
    (even if the light curve's no thing of beauty).
    
    Two new (relatively) bright northern targets.  The first is LD 317
    ("And"), a rewarding 14.5 mag star which we started last year and seemed
    to find 5 hr and 25 minute modulations.  These demand more study!  The
    second is LQ Peg, of similar brightness and unknown period.  Our past
    efforts on LQ Peg have been meager and unsuccessful - and so, for that
    matter, has everyone else's.
    
    And in the south...
    
    We had quit on RZ Gru... but then the star started to dive down to a low
    state, and that enormously boosts its priority (because it's rare that we
    get to observe these things with advance notice).  So RZ Gru, presently
    hanging near 14th magnitude, is now a very good target for long
    time-series coverage.
    
    As is BW Scl.  In that one (about 16.5-17) we're mainly interested in the
    orbital signal, although anything else would be a bonus - and an outburst
    would be gold (none recorded in history, although it's very likely to be a
    dwarf nova).
    
    So there's the new menu.  Happy observing!  Beautiful fall weather has
    finally struck in the northeast US - I hope it's as fine where you are.
    
    joe
    
    Received on 29 Sep 2005