3D Simulations of the Fragmentation of Photoevaporating Clumps Embedded in a Stellar Wind

Details 3D Simulations of the Fragmentation of Photoevaporating Clumps Embedded in a Stellar Wind 3D Simulations of the Fragmentation of Photoevaporating Clumps Embedded in a Stellar Wind

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005rmxaa..41...45r&link_type=abstract

Revista Mexicana de Astronomía y Astrofísica Vol. 41, pp. 45-55 (2005) (http://www.astroscu.unam.mx/~rmaa/)

Astronomy and Astrophysics

Astronomy

11

Ism: Hregions, Ism: Kinematics And Dynamics, Ism: Planetary Nebulae

Scientific paper

We present 3D numerical simulations of the interaction of a dense, neutral clump with an impinging external wind+ionizing photon field. We find that models with very weak ionizing photon fields produce clumps that fragment as the time evolution proceeds, in agreement with previous clump/wind interaction models. Models with stronger ionizing photon fields present less fragmentation, and for strong enough photon fields only a single, dense condensation is produced.

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