ASIAA Computational Astrophysics at ASIAA
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Seminar

2017-03-10
Progress report meeting
CompAS members (ASIAA) R1108
2017-03-01
There Is Life after Stellar Middle Age
Paul Ricker (University of Illinois at Urbana-Champaign) R1108
2017-01-16
Pattern speeds in galaxies
Daniel Pfenniger (University of Geneva) R1108
2017-01-09
Winds from black hole accretion systems
Defu Bu (SHAO) R1108
2016-12-16
Save the Planet, Feed the Star: How Planets can Survive Migration and Drive Accretion
Jeffrey Fung (Berkeley) R1108
2016-12-09
Selected topics in theoretical astrophysics
Min-Kai Lin (ASIAA) R1108
2016-12-02
Hydrodynamic processes in protoplanetary accretion disks
Min-Kai Lin (ASIAA) R1108
2016-10-14
Self-consistent Neutrino-Driven Core-Collapse Supernova Simulations with Neutrino Transport
Kuo-Chuan Pan (University of Basel) R1108
2016-08-08
Astrochemistry: gas-phase chemical network
Hideko Nomura (Tokyo Institute of Technology) R1108
2016-08-08
Gas-grain astrochemical models: challenge and hints to improve the solid part
Patrice Theulé (Aix-Marseille University) R1108

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History of CFD-MHD initiative

CFD-MHD initiative has been a joint research project of the Institute of Astronomy and Astrophysics (ASIAA) and the Institute of Mathematics (ASIM) of the Academia Sinica, and the Department of Mathematics of the National Taiwan University. In February 2012, the name of the initiative, CFD-MHD, was changed into CompAS, for Computational Astrophysics.

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Simulations vs Observations(NGC 6782).
The CompAS (formerly CFD-MHD) team is developing a high performance numerical code to study the structure formation in disk galaxies. Numerical simulations have successfully reproduced the spiral arms excited by stellar bars, such as the ones seen in NGC 6782

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