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Modeling the Spectral Signatures of Accretion Disk Winds: A New Monte Carlo Approach
Long & Knigge 2002 The Astrophysical Journal 579 725.
Caption: Fig. 2.
Cartoon of the wind description employed by KWD95. The wind is symmetric with respect to the disk.
© 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
