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We present results of 2-dimensional calculations of a supernova remnant expansion into a cloudy medium. We use direct single fluid simulation of a multiphase interstellar medium. We find some disagreements between our numerical results and theoretical predictions by White and Long (1991): the X-ray map does not reveal the property of centrally peaked luminosity of the remnant.
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Keywords: Hydrodynamics; Interstellar medium; Shock waves; Supernova remnants

Document Type: Research Article

Affiliations: Department of Physics, Volgograd State University, 2ya Prodol'naya, 30, Volgograd 400062, Russia

Publication date: 01 January 2002

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