2011 International Summer Institute for Modeling in Astrophysics

Parent: International Summer Institute for Modeling in Astrophysics

eScholarship stats: Breakdown by Item for January through April, 2025

ItemTitleTotal requestsDownloadView-only%Dnld
0r71s3v9Detecting the earliest stages of giant planet formation in scattered light434399.3%
4707m4sxOhmic dissipation in hot Jupiters3142712.9%
96m3847fAnalytical studies of fragmentation during gravitational collapse2762122.2%
0bx48606Planetary dynamics in collisional particle disks252238.0%
3813j8hbAbundance and evolution of gas around Beta Pictoris2451920.8%
4461g8ghGap formation in transitional and pre-transitional disks: dust filtration in the presence of coagulation and fragmentation.232218.7%
06k8s8bwDestroying resonance between Neptune and its resonant Kuiper Belt Objects by stochastic planetesimal scatterings2131814.3%
1kt0k72gConvectively generated zonal jets by thunderstorms on Jupiter2131814.3%
7n09f14xImproving the grain growth model in the outer part of circumstellar disks2161528.6%
3p74t14xA simple model for understanding the day-night temperature constrast on Hot Jupiters2031715.0%
0xc2c5w6Multi-phase turbulent ISM: Theory Confronting Observations1751229.4%
35s753p6Disk Dynamos in Simulations of Collapsing Cores1741323.5%
7f43z58pDay-night cold traps for TiO in hot Jupiter atmospheres1741323.5%
7m77v9sdCharge exchange in the colliding winds of Hot Jupiters and their host stars1641225.0%
4v42t9t6Planetesimal formation: shear instabilities at the dust-rich mid-plane1421214.3%

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