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Dynamical Expansion of Ionization and Dissociation Front around a Massive Star. II. On the Generality of Triggered Star Formation
Takashi Hosokawa, Shu-ichiro Inutsuka
We analyze the dynamical expansion of the HII region, photodissociation region, and the swept-up shell, solving the UV- and FUV-radiative transfer, the thermal and chemical process…
Can WNM survive inside Molecular Clouds ?
P. Hennebelle, S. Inutsuka
Recent high resolution numerical simulations have suggested that the interstellar atomic hydrogen clouds have a complex two-phase structure. Since molecular clouds form through the…
Self-Sustained Ionization and Vanishing Dead Zones in Protoplanetary Disks
Shu-ichiro Inutsuka, Takayoshi Sano
We analyze the ionization state of the magnetohydrodynamically turbulent protoplanetary disks and propose a new mechanism of sustaining ionization. First, we show that in the quasi…
Making the corona and the fast solar wind: a self-consistent simulation for the low-frequency Alfven waves from photosphere to 0.3AU
Takeru K. Suzuki, Shu-ichiro Inutsuka
We show that the coronal heating and the fast solar wind acceleration in the coronal holes are natural consequence of the footpoint fluctuations of the magnetic fields at the photo…