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    National Tsing Hua University Institutional Repository > 歷任校長 > 徐遐生 (2002-2006) > 期刊論文 >  GAS-DYNAMICS OF SEMIDETACHED BINARIES .2. VERTICAL STRUCTURE OF THE STREAM


    Please use this identifier to cite or link to this item: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/81028


    Title: GAS-DYNAMICS OF SEMIDETACHED BINARIES .2. VERTICAL STRUCTURE OF THE STREAM
    Authors: LUBOW, S.H.;SHU, F.H.
    教師: 徐遐生
    Date: 1976
    Publisher: American Astronomical Society
    Relation: ASTROPHYSICAL JOURNAL, American Astronomical Society, Volume 207, Issue 1, 1976, Pages L53-L55
    Keywords: BINARY STARS
    GAS DYNAMICS
    GRAVITATIONAL FIELDS
    X RAY ASTRONOMY
    X RAY STARS
    GRAVITATIONAL EFFECTS
    STELLAR GRAVITATION
    STELLAR MASS
    X RAY SOURCES
    Abstract: The letter considers the three-dimensional dynamics of the stream in semidetached binaries undergoing Roche-lobe overflow. Results of an earlier communication are generalized to include the dynamic effects in the direction perpendicular to the orbital plane. It is found that the scale height of the stream characteristically exceeds its corresponding hydrostatic value by a significant factor because the inertia of the gas prevents it from responding instantaneously to the changing gravitational field. This effect is important for the interpretation of observations relating to stream-disk impacts in cataclysmic variables and in binary X-ray sources of low total mass.
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    Relation Link: http://aas.org/
    URI: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/81028
    Appears in Collections:[ 徐遐生 (2002-2006)] 期刊論文
    [物理系] 期刊論文

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