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Miller, Schlaufman, and LaughlinUCSC Astronomy FLASH 4132007
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waves result from planet-disk interactions at Lindblad resonances. ... that the planet will migrate relative to the disk at a rate ... – PowerPoint PPT presentation
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Title: Miller, Schlaufman, and LaughlinUCSC Astronomy FLASH 4132007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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We use the 2D hydrodynamics code described in
Laughlin et al. (1996)
Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Angular momentum is transfered as the mode moves
outward
Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Net angular impulse transfer for undamped and
damped modes depends on angle with respect to the
planet
Average Impulse is -0.0026 and -0.0029
respectively
Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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Miller, Schlaufman, and Laughlin UCSC
Astronomy FLASH 4/13/2007
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