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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. 8.

Calculated spectrum for the fiducial SV93 geometry, which has ﹩\dot{m}_{\mathrm{disk}\,}﹩ of 10−8 ﹩M_{\odot }﹩ yr−1 and ﹩\dot{m}_{\mathrm{wind}\,}﹩ of 10−9 ﹩M_{\odot }﹩ yr−1 as a function of inclination angle. In contrast to Fig. 7, here the disk and WD were simulated in terms of appropriately weighted Hubeny (1988) model atmospheres.

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