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Magneto-Hydrodynamic simulations on galaxy modeling

Published online by Cambridge University Press:  10 June 2020

Wei-Chen Wang  and
Ke-Jung Chen
Wei-Chen Wang
Affiliation:
Academia Sinica Institute of Astronomy and Astrophysics, National Taiwan University email: weichenwang.network@gmail.com
Ke-Jung Chen
Affiliation:
Academia Sinica Institute of Astronomy and Astrophysics, ASMAB R1420, No.1, Sec.4, Roosevelt Rd, Taipei10617, Taiwan, R.O.C. email: kjchen@asiaa.sinica.edu.tw
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Abstract

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Magnetic field plays an important role in star formation and galaxy evolution. Previous studies discussed about the origin of magnetic field and its effect to the environment. With the recent advancement of supercomputers, adding the magnetic field to a cosmological hydrodynamic simulations only become feasible. In this proceeding, we present the results of high-resolution magneto-hydrodynamic simulation with GIZMO and compare our simulation result with the previous literature and the observations.

Keywords

galaxies: evolutiongalaxies: magnetic fieldsmethods: n-body simulations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S341: Challenges in Panchromatic Modelling with Next Generation Facilities , November 2019 , pp. 320 - 322
Copyright
© International Astronomical Union 2020

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