SETI public: 4,131 stars within 33 parsecs of Sol

From: LARRY KLAES (ljk4_at_msn.com)
Date: Thu Jun 09 2005 - 03:41:30 PDT

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    Paper: astro-ph/0506152
    Date: Tue, 7 Jun 2005 20:43:27 GMT (762kb)

    Title: Nearby stars from the LSPM-north Proper Motion Catalog. I. Main
    Sequence
      Dwarfs and Giants Within 33 Parsecs of the Sun

    Authors: Sebastien Lepine
    Comments: 13 pages, accepted for publication in the Astronomical Journal
    \\
      A list of 4,131 dwarfs, subgiants, and giants located, or suspected to be
    located, within 33 parsecs of the Sun is presented. All the stars are drawn
    from the new LSPM-north catalog of 61,976 stars with annual proper motions
    larger than 0.15''/yr$. Trigonometric parallax measurements are found in the
    literature for 1,676 of the stars in the sample; photometric and
    spectroscopic
    distance moduli are found for another 783 objects. The remaining 1,672
    objects
    are reported here as nearby star candidates for the first time. Photometric
    distance moduli are calculated for the new stars based on the (M_V,V-J)
    relationship, calibrated with the subsample of stars which have
    trigonometric
    parallaxes. The list of new candidates includes 539 stars which are
    suspected
    to be within 25 parsecs of the Sun, including 63 stars estimated to be
    within
    only 15 parsecs. The current completeness of the census of nearby stars in
    the
    northern sky is discussed in light of the new candidates presented here. It
    is
    estimated that 32% (18%) of nuclear burning stars within 33 parsecs (25
    parsecs) of the Sun remain to be located. The missing systems are expected
    to
    have proper motions below the 0.15''/yr limit of the LSPM catalog.

    \\ ( http://arXiv.org/abs/astro-ph/0506152 , 762kb)


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