Ionization Front Instabilities

Details Ionization Front Instabilities Ionization Front Instabilities

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..184w&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

3

H Ii Regions, Ism: Kinematics And Dynamics, Planetary Nebulae

Scientific paper

Resolved photoionized nebulae, such as H II regions and planetary nebulae, have complex and dynamic structures, but the origin and evolution of these structures remain controversial: is it the result of inhomogeneity in the upstream gas, or intrinsic instability of the shock and ionization front surrounding the region? I describe numerical and analytic work which investigates the stability of ionization fronts, aiming to help resolve these questions.

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