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    RZ LMi erupts

    From: Joe Patterson <jop_at_astro.columbia.edu>
    Date: Sun, 23 Dec 2001 21:40:43 -0500 (EST)
    Dear CBAers,
    
    Well, Gary Poyner reported RZ LMi at 13.9 last night, very likely a
    superoutburst (judging from the brightness and the time since the last
    one).  Even though this star utterly conflicts with BK Lyn, it belongs
    right there with BK Lyn in priority (tops in the after 10 p.m. category).
    There are several reasons we want to really focus on this star:
    (1) Porb still hasn't been measured, and it's an important one;
    (2) In a previous year the superhumps appeared to remember phase from one
        superoutburst to the next, muy interesante.
    (3) As the most frantic of the H-rich dwarf novae, RZ LMi gives the
        maximum leverage per night invested - to study the detailed properties
        of superhumps (in other words, the show's beginning, middle, and end
        can be conveniently covered)
    
    Still, BK Lyn may be the better target for the next 3 days, when Cindy
    Taylor will be covering it with spectroscopy.  If you're feeling virtuous,
    do 'em both!  Otherwise select one and stick with it - both will reward
    your effort.
    
    By the way it's best to start on 'em as soon as you can get 'em, even if
    that means ignoring or cutting short FS Aur.  These are time-critical
    observations, and FS can wait a bit.
    
    Anyone doing EC0511-79 down south?  By the way, we're gearing up for a TX
    Col campaign in early January, which Dave Buckley will coordinate from
    South Africa.  That's a mighty good one too (now - and then it will be el
    primo in early January).  We'll have a chart up in a few days, but you can
    find one in the on-line ("living") Downes-Shara CV catalog.
    
    joe
    
    Received on 23 Dec 2001