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Keywords

HYDRODYNAMICS
ISM: H II REGIONS
SHOCK WAVES
SUPERNOVA REMNANTS

How to Cite

Photoionizing Shocks in the ISM. (2001). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 10(1), 49-52. https://astronomia.unam.mx/journals/rmxac/article/view/2001rmxac..10...49a
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Abstract

We investigate the ionization structure of precursor ion{H}{2} regions formed around supernova remnants (SNR) by means of radiation-hydrodynamic calculations that include a detailed treatment of the non-equilibrium ionization both within the SNR and in the ionized precursor region. A qualitative comparison is made with observations of the Large Magellanic Cloud SNR N132D.