Fig. 7 from Modeling the Spectral Signatures of Accretion Disk Winds: A New Monte Carlo Approach

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Modeling the Spectral Signatures of Accretion Disk Winds: A New Monte Carlo Approach

Authors: Knox S. Long and Christian Knigge

Long & Knigge 2002 The Astrophysical Journal 579 725.

Provider: AAS Journals

Caption: Fig. 7.

Calculated spectrum for the fiducial SV93 geometry as observed at an inclination of 62﹩\fdg﹩5 and assuming that both the disk and the WD radiate as blackbodies.

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