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Reprocessing in Luminous Disks

  • Authors: K. R. Bell

Bell 1999 The Astrophysical Journal 526 411.

  • Provider: AAS Journals

Caption: Fig. 10.

Detailed model in quiescence. (a) Relative disk thickness as a function of radial position. (b) Temperature profiles. Surface temperatures of detailed model over five iterations (solid lines), initial, accretion‐only surface temperatures (dashed line), and midplane temperatures for unilluminated models with ﹩\alpha =10^{-4}﹩ and ﹩10^{-2}﹩ (dot‐dashed lines, upper and lower respectively). (c) Spectral energy distributions. Star (asterisks), detailed model, final iteration (solid line) and accretion only (dashed line).

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