Image Details

Choose export citation format:

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. 9.

Comparison between the HUT spectrum of Z Cam (black) and a model spectrum (gray) calculated using a prescription for the wind geometry similar to that suggested by Knigge et al. (1997). The model has been smoothed slightly to reflect the resolution of HUT. Some of the stronger lines, including the Lyman series of H, are labeled. The regions near strong features at 1304 and 1356 Å may have been affected by airglow lines.

Other Images in This Article
Copyright and Terms & Conditions