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Digitale Medien

Flows in clumpy planetary nebulae (1996)

Hartquist, T. W. ; Dyson, J. E.

Springer

Astrophysics and space science 245 (1996), S. 263-273

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ISSN: 1572-946X

Schlagwort(e): Planetary nebulae ; Hydrodynamics ; Multi-phase flows

Quelle: Springer Online Journal Archives 1860-2000

Thema: Physik

Notizen: Abstract The dynamics of clumps observed in planetary nebulae are considered. The possibility that SiO maser spots in evolved stars and the planetary nebula clumps are formed by the Parker instability behind shocks in pulsating stars' atmospheres is raised. Molecular observations of the clumps are suggested. The effects of the ablation of clumps on the global flow structure of a more tenuous plasma in which they are embedded are reviewed.

Materialart: Digitale Medien

URL: http://dx.doi.org/10.1007/BF00642231

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