SETI public: More "Sol" Brothers

From: LARRY KLAES (ljk4_at_msn.com)
Date: Thu Jun 30 2005 - 06:42:58 PDT

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    Paper: astro-ph/0506733
    Date: Wed, 29 Jun 2005 17:09:11 GMT (659kb)

    Title: The Solar Neighborhood XV: Discovery of New High Proper Motion Stars
    with mu >= 0.4"/yr between Declinations -47 degrees and 00 degrees

    Authors: John P. Subasavage (1), Todd J. Henry (1), Nigel C. Hambly (2),
    Misty
    A. Brown (1), Wei-Chun Jao (1), Charlie T. Finch (1)((1) Georgia State
    University, (2) Institute for Astronomy, University of Edinburgh)
    Comments: 36 pages, 5 figures, accepted for publication in Astronomical
    Journal
    \\
    We report the discovery of 152 new high proper motion systems (mu >=
    0.4"/yr)
    in the southern sky (Declination = -47 degrees to 00 degrees) brighter than
    UKST plate R_{59F} =16.5 via our SuperCOSMOS-RECONS (SCR) search. This paper
    complements Paper XII in The Solar Neighborhood series, which covered the
    region from Declination = -90 degrees to -47 degrees and discussed all 147
    new
    systems from the southernmost phase of the search. Among the total of 299
    systems from both papers, there are 148 (71 in Paper XII, 77 in this paper)
    new
    systems moving faster than 0.5"/yr that are additions to the classic ``LHS''
    (Luyten Half Second) sample. These constitute an 8% increase in the sample
    of
    all stellar systems with mu >= 0.5"/yr in the southern sky.
    As in Paper XII, distance estimates are provided for the systems reported
    here based upon a combination of photographic plate magnitudes and 2MASS
    photometry, assuming all stars are on the main sequence. Two SCR systems
    from
    the portion of the sky included in this paper are anticipated to be within
    10
    pc, and an additional 23 are within 25 pc. In total, the results presented
    in
    Paper XII and here for this SCR sweep of the entire southern sky include
    five
    new systems within 10 pc and 38 more between 10 and 25 pc. The largest
    number
    of nearby systems have been found in the slowest proper motion bin, 0.6"/yr
    >
    mu >= 0.4"/yr, indicating that there may be a large population of low proper
    motion systems very near the Sun.

    \\ ( http://arXiv.org/abs/astro-ph/0506733 , 659kb)


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