SETI public: Constraints on Inner Disk Evolution Timescales: A Disk Census of the eta Chamael

From: LARRY KLAES (ljk4_at_msn.com)
Date: Thu Jun 16 2005 - 07:29:54 PDT

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    Paper: astro-ph/0506352
    Date: Wed, 15 Jun 2005 17:18:01 GMT (22kb)

    Title: Constraints on Inner Disk Evolution Timescales: A Disk Census of the
    eta
    Chamaeleontis Young Cluster

    Authors: Karl E. Haisch Jr. (UVSC), Ray Jayawardhana (Toronto) and Joao
    Alves
    (ESO)
    Comments: accepted for publication in Astrophysical Journal Letters
    \\
    We present new L' (3.8-micron) observations of stars in the nearby (~97 pc)
    young (~6 Myr) compact cluster around eta Chamaeleontis, obtained with the
    European Southern Observatory's Very Large Telescope in Paranal, Chile. Our
    data, combined with J,H, Ks photometry from the 2-Micron All Sky Survey,
    reveal
    that only two of the 12 members surveyed harbor L'-band excesses consistent
    with optically thick inner disks; both are also likely accretors.
    Intriguingly,
    two other stars with possible evidence for on-going accretion, albeit at
    very
    low rates, do not show significant infrared excess: this may imply
    substantial
    grain growth and/or partial clearing of the inner disk region, as expected
    in
    planet formation scenarios. Our findings suggest that eta Cha stars are in
    an
    epoch when disks are rapidly evolving, perhaps due to processes related to
    planet building, and provide further constraints on inner disk lifetimes.

    \\ ( http://arXiv.org/abs/astro-ph/0506352 , 22kb)


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