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X-ray Photoevaporation-Starved T Tauri Accretion

  • Authors: Jeremy J. Drake, Barbara Ercolano, Ettore Flaccomio, and Giusi Micela

DRAKE et al. 2009 The Astrophysical Journal 699 L35.

  • Provider: AAS Journals

Caption: Figure 1.

X-ray heating-induced photoevaporation rate, , from a 2D protoplanetary disk model expressed as a function of the model coronal X-ray luminosity of the central star, L X , computed using the mocassin program (see the text and Ercolano et al. 2008a for details).

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