National Tsing Hua University Institutional Repository:Protostellar X-rays, jets, and bipolar outflows
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    NTHUR > Presidents > Shu, Frank Hsia-San (2002-2006 ) > SFHS Conference papers >  Protostellar X-rays, jets, and bipolar outflows


    Please use this identifier to cite or link to this item: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/80901


    Title: Protostellar X-rays, jets, and bipolar outflows
    Authors: Shu, FH;Shang, H
    Teacher: 徐遐生
    Date: 1997
    Publisher: Kluwer
    Relation: 182nd Symposium of the International-Astronomical-Union on Herbig-Haro Flows and the Birth of Low Mass Stars, CHAMONIX, FRANCE, JAN 20-26, 1997
    Keywords: MAGNETOCENTRIFUGALLY DRIVEN FLOWS
    T-TAURI STARS
    YOUNG STARS
    ACCRETION DISKS
    WINDS
    MASS
    COLLIMATION
    MODELS
    REGION
    Abstract: We review the theory of x-winds in young stellar objects (YSOs). In particular, we consider how a model where the central star does not corotate with the inner edge of the accretion disk may help to explain the enhanced emission of X-rays from embedded protostars. We argue, however, that the departure from corotation is not large, so a mathematical formulation that treats the long-term average state as steady and axisymmetric represents a useful approximation. Magneto centrifugally driven x-winds of this description collimate into jets, and their interactions with the surrounding molecular cloud cores of YSOs yield bipolar molecular outflows.
    Accession Number: WOS:A1997BJ28R00019
    Relation Link: http://adsabs.harvard.edu/abs/1997IAUS..182..225S
    http://www.springer.com/?SGWID=5-102-0-0-0
    URI: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/80901
    Appears in Collections:[Shu, Frank Hsia-San (2002-2006 )] SFHS Conference papers
    [Department of Physics] PHYS Conference Papers

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