Bi stability - PowerPoint PPT Presentation

Modeling Disks of sgB[e] Stars

Modeling Disks of sgB[e] Stars. Jon E. Bjorkman Ritter Observatory. Dusty Hot Star Winds. Hot stars with dust : B[e] WR Novae and Supernovae Wind must cool below condensation temperature Dust forms at large distances

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LECTURE 11 - THE OP-AMP

LECTURE 11 - THE OP-AMP. Op-Amp: “Operational Amplifier” Circuit Symbol:. Reality:. Differential Amplifier. Circuit Model in linear region. V 0. V +. +. A. AV 1. R i. . V . +. . +. +. V 1. V 0. But if A ~ , is the output infinite?. “Very high gain” . . .

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