Titlebook: Astrophysical and Laboratory Plasmas; A Festschrift for Pr A. J. Willis,T. W. Hartquist Book 1996 Springer Science+Business Media Dordrecht

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Using an Animation and Effects Library,ing of material between different nuclear burning zones in evolved stars and turbulent boundary layers (which are present in and influence the structures and evolution of all diffuse astrophysical sources) are treated.

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Foundation ActionScript 3.0 Image Effectshat self-consistent models of the dynamical and chemical evolution of collapsing cores, coupled to multiple high resolution line observations, will provide definitive evidence for the presence of infall in these objects.

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The Chromosphere-Corona Transition Region in Late-Type Starsof stellar transition regions show common behaviour as well as systematic trends. The basic methods used in making models of the transition region are set out. Observations relating to inhomogeneities in the solar transition region are summarized. The structure and energy balance of stellar transition regions and the trends emerging are discussed.

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