Lecture 16: Winds, Jets and Outflows
Lecture 16: Winds, Jets and Outflows
Lecture 16: Winds, Jets and Outflows
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Photoevaporation of disks(Very brief)Ionization of disk surface creates surface layer of hot gas. Ifthis temperature exceeds escape velocity, then surfacelayer evaporates.v esc≈ GM 1/ 2⎛⎛ ⎞⎞⎜⎜ ⎟⎟⎝⎝ r ⎠⎠Evaporation proceeds for radii beyond:€r ≥ GM ≡ r2 grc sHII