Clouds and Instabilities in Supernova Remnant Structure: Interstellar Turbulence and Rippled Shocks

Details Clouds and Instabilities in Supernova Remnant Structure: Interstellar Turbulence and Rippled Shocks Clouds and Instabilities in Supernova Remnant Structure: Interstellar Turbulence and Rippled Shocks

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..258r&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

1

Shock Waves, Supernova Remnants, Turbulence

Scientific paper

The beautiful spherical blastwaves of theory are disrupted by interaction with density inhomogeneities and by thermal and dynamical instabilities. Various tricks, involving either Doppler shift velocities or model assumptions, make it possible to construct a 3-D picture of the structure from a 2-D image. This paper will discuss the expected nature of the density inhomogeneities and the consequences for the appearance of an SNR, along with the conditions for some instabilities, and it will present an example of attempts to sort it all out and discuss the role of interstellar turbulence.

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