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    New stars for 2006

    From: Joe Patterson <jop_at_astro.columbia.edu>
    Date: Thu, 29 Dec 2005 17:26:01 -0500 (EST)
    Dear CBAers,                                                 12/29/05
    
    After the onslaught of final exams and letters to write, I've done the
    first-pass evaluation of this month's targets.  And it's time for a
    complete revamping of the menu.
    
    HT Cam and V701 Tau were eruptive stars, and are gone.  WX Hyi and VW Hyi
    are at quiescence; we have good hump timings and can update the
    ephemerides accordingly.  Probably time to shift away from these stars -
    unless one of 'em jumps into supermax in the next week.
    
    Tau 2 seems to now be in an intermediate state - very annoying for period
    search, and indeed for any kind of study.  Suspended temporarily.
    
    FS Aur stays viable - as it always will until we figure out its strange
    period structure.  But the period is stable... so let's let it go till
    late in the season.
    
    My all-sky recommendations are two: SDSS 0407-06 ("Eri") and V1193 Ori.
    Both are nicely astride the celestial equator, transiting near midnight,
    and have reported superhump signals in their light curves.  We've never
    seen 'em - but then again, we've never looked!  We need to, in order to
    evaluate these important reports.  Let's get all feasible continents going
    on this!  V1193 Ori is about 14.1, an easy target.  Eri is much fainter,
    but has nice deep eclipses to reward your efforts.
    
    And two other stars of a distinctly southern preference.  There's the
    immortal T Pyx.  We do it every year, tracking its mysterious and enormous
    period increase.  I promise this is the last!  A few weeks of timings, and
    the study is finished (and I'll write it up forthwith).  And there's AQ
    Men = EC0511-7955.  We've only observed that one year... but one more
    year, or likely just one month, will wrap up the study.
    
    And two northern stars too.  Early in the night, there's "Cam" =
    HS0506+77.  A newly discovered VY Scl star, definitely ripe for superhump
    search; usually at 15-15.5, but with occasional low states.  And DW Cnc:
    a nice discovery of 2 years ago, we need to follow up (for the next month
    at least) to measure the long-term period change.
    
    That's the new menu. Happy observing!
    
    By the way, let me know if you're considering coming to CA for the SAS/CBA
    meeting in late May.
    
    joe
    
    Received on 29 Dec 2005