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Reprocessing in Luminous Disks

  • Authors: K. R. Bell

Bell 1999 The Astrophysical Journal 526 411.

  • Provider: AAS Journals

Caption: Fig. 8.

Spectral energy distribution (top panel) and temperature profile (bottom panel) of ﹩z=9/8﹩ model broken down to show relative contribution of various components. Heavy lines: total result; asterisks (in SED only): stellar contribution; dashed lines: locally generated by accretion processes; dotted lines: stellar reprocessing contribution; thin solid lines: disk‐to‐disk reprocessing component.

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