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Critical Magnetic Field Strength for Suppression of the Richtmyer-Meshkov Instability in Plasmas
Takayoshi Sano, Tsuyoshi Inoue, Katsunobu Nishihara
The critical strength of a magnetic field required for the suppression of the Richtmyer-Meshkov instability (RMI) is investigated numerically by using a two-dimensional single-mode…
Thermal Instability behind a Shock Wave in HI and Molecular Clouds
Takuhiro Aota, Tsuyoshi Inoue, Yuri Aikawa
We performed one-dimensional hydrodynamic simulations with detailed cooling, heating and chemical processes to examine the thermal stability of shocked gas in cold neutral medium (…
Origin of Radially Aligned Magnetic Fields in Young Supernova Remnants
Tsuyoshi Inoue, Jiro Shimoda, Yutaka Ohira +1
It has been suggested by radio observations of polarized synchrotron emissions that downstream magnetic field in some young supernova remnants are oriented radially. We study magne…
Formation of Massive Molecular Cloud Cores by Cloud-cloud Collision
Tsuyoshi Inoue, Yasuo Fukui
Recent observations of molecular clouds around rich massive star clusters including NGC3603, Westerlund 2, and M20 revealed that the formation of massive stars could be triggered b…