Clumpy Flows in Protoplanetary and Planetary Nebulae

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dc.creatorPoludnenko, A. Y.
dc.creatorFrank, A.
dc.creatorMitran, S.
dc.date2003-10-10
dc.date.accessioned2026-07-07T02:10:18Z
dc.date.available2026-07-07T02:10:18Z
dc.descriptionMany astrophysical flows occur in inhomogeneous media. We briefly discuss some general properties of the adiabatic and radiative inhomogeneous systems and discuss the relevance of those properties to the planetary nebulae systems. We then focus on radiative hypersonic bullets and the applicability of this model to planetary and protoplanetary systems such as CRL 618, NGC 6543, Hen 3-1475.
dc.description4 pages, 2 figures. To appear in "Asymmetric Planetary Nebulae III", eds. M. Meixner, J. Kastner, N. Soker and B. Balick, 2004, ASP Conference Series, for higher resolution version and animations see http://www.pas.rochester.edu/~wma
dc.identifierhttps://arxiv.org/abs/astro-ph/0310286
dc.identifierhttp://arxiv.org/abs/astro-ph/0310286
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6695
dc.subjectAstrophysics
dc.titleClumpy Flows in Protoplanetary and Planetary Nebulae
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