Computational Astrophysics at ASIAA

Web Name: Computational Astrophysics at ASIAA

WebSite: http://compas.asiaa.sinica.edu.tw

ID:237503

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Astrophysics,Computational,ASIAA,at,

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>> ASIAA HomeHistory Research PeoplePublicationFacility Seminar 2017-12-18The Parabolic Jet from the Spinning Black Hole in M87Masanori Nakamura (ASIAA) R11072017-12-15The most powerful transients in 3DPhilipp Moesta (Berkeley) R11082017-08-16New Ways of Studying Magnetic Fields: Implications of MHD Turbulence TheoryAlexandre Lazarian (University of Wisconsin, Madison) R11072017-08-09Galactic Outflows and Extended Narrow-line Regions in Luminous Obscured AGNAi-Lei Sun (ASIAA) R11082017-08-03The masses of feature-producing planets in protoplanetary disksRuobing Dong (University of Arizona) R11082017-08-02Physical and Chemical Structure of Protoplanetary DisksHideko Nomura (Tokyo Institute of Technology) R11082017-08-01Ice and firePatrice Theulé (University of Aix Marseille) R11082017-07-28Six Decades of Spiral Density Wave TheoryFrank H. Shu (ASIAA, and Astron Solutions Corporation) 1F Auditorium2017-07-27Rings and gaps, but no planets ?Chunhua Qi (Harvard-Smithsonian Center for Astrophysics) R11072017-07-27AMRPak-Shing Li (University of California, Berkeley) R1107

(more...)

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.


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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Last Updated: 2017-01-12 | Privacy and Security Policy | Contact: webasiaa.sinica.edu.tw

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