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A Supernova Remnant Collision with a Stellar Wind - IOPscience

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A Supernova Remnant Collision with a Stellar Wind

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© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Pablo F. Velázquez et al 2003 ApJ 584 284 DOI 10.1086/345663

0004-637X/584/1/284

Abstract

Numerical simulations of the interaction between supernova ejecta and a stellar wind are presented. We follow the temporal evolution of the shock fronts that are formed through such an interaction and determine the velocities, temperatures, and densities. We model the X-ray emission from the supernova remnant-stellar wind collision region, and we compare it with recent results from X-ray observations carried out with the Chandra satellite of the SMC supernova remnant SNR 0057-7226, which could be interacting with the wind of the Wolf-Rayet system HD 5980. The simulations predict the presence of shell-like regions of enhanced X-ray emission that are consistent with the presence of X-ray-emitting arcs in the Chandra image. Also, the observed X-ray luminosity is comparable to the X-ray luminosities we obtain from the simulations for a supernova with an initial energy in the (1–5) × 1050 ergs range.

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10.1086/345663