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Radiative Instabilities in Simulations of Spherically Symmetric Supernova Blast Waves
Kimoto & Chernoff 1997 The Astrophysical Journal 485 274.
Caption: Fig. 5.
Shock velocity for ISM density nH = 0.1 for calculation using hard‐sphere interior boundary condition.
© 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
