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    National Tsing Hua University Institutional Repository > 歷任校長 > 徐遐生 (2002-2006) > 期刊論文 >  ON THE ROLE OF PHOTOSPHERIC CONVECTION IN W-URSAE MAJORIS STARS


    Please use this identifier to cite or link to this item: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/81023


    Title: ON THE ROLE OF PHOTOSPHERIC CONVECTION IN W-URSAE MAJORIS STARS
    Authors: ANDERSON, L.;SHU, F.H.
    教師: 徐遐生
    Date: 1978
    Publisher: American Astronomical Society
    Relation: ASTROPHYSICAL JOURNAL, American Astronomical Society, Volume 221, Issue 3, 1978, Pages 926-928
    Keywords: CONVECTIVE FLOW
    ECLIPSING BINARY STARS
    PHOTOSPHERE
    STELLAR ATMOSPHERES
    LIGHT CURVE
    LIMB DARKENING
    RADIATIVE TRANSFER
    Abstract: We correct the derivation of the source function in the atmospheres of contact binaries given in an earlier communication by Anderson and Shu. This correction affects the cases when convection is present in the photosphere. In our new treatment photospheric convection is more efficient for reducing limb darkening. This result does not, however, modify the numerical examples considered in our earlier paper.
    Relation Link: http://aas.org/
    URI: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/81023
    Appears in Collections:[ 徐遐生 (2002-2006)] 期刊論文
    [物理系] 期刊論文

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