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Expanding shells: instability with non-linear terms

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    0124838 - ASU-R 20010091 RIV US eng C - Conference Paper (international conference)
    Wünsch, Richard - Palouš, Jan
    Expanding shells: instability with non-linear terms.
    Dynamics of star clusters and the Milky way. San Francisco: Astronomical Society of the Pacific, 2001 - (Deiters, S.; Fuchs, B.; Just, A.; Spurzem, R.; Wielen, R.), s. 557-559. ASP Conference series., 228.
    [Dynamics of star clusters and the Milky way. Heidelberg (DE), 20.03.2000-24.03.2000]
    R&D Projects: GA AV ČR KSK1003601
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : formation * ISM * structure * galaxy * evolution
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    A model of the thin shell expanding into a uniform ambient medium is developed. Density perturbations are described using equations with linear and quadratic terms and the linear and the nonlinear solutions are compared. The interaction of modes on the shell surface is discussed defining the rime when the fragments are formed.
    Permanent Link: http://hdl.handle.net/11104/0023097


     
     

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