X-ray and IR Signatures of Dusty Adiabatic Shock Waves

Details X-ray and IR Signatures of Dusty Adiabatic Shock Waves X-ray and IR Signatures of Dusty Adiabatic Shock Waves

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...189.5502v&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #55.02; Bulletin of the American Astronomical Society, Vol. 28, p.1345

Astronomy and Astrophysics

Astronomy

Scientific paper

We have previously constructed a steady-state dusty shock model which is a self-consistent treatment of the effects of destruction, thermal heating, and deceleration of the grains on the gas-phase abundances, ionization structure and X-ray emission. We have now adapted the code to predict emissions from a dusty adiabatic blast wave. We make specific predictions about the X-ray spectrum and thermal IR grain emissions emanating from the postshock material. We will compare these new predictions to approximations adapted from the steady-state modeling. We will also compare to global observations of primary shocks in the Cygnus Loop and Puppis A SNRs in an effort to broaden our understanding of dusty shocks and remnant evolution.

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