Hydrodynamic simulation of the Galactic disc: Radial migration of the early Solar system by giant molecular clouds
Fujimoto, Inutsuka & Baba (2023)
Radial migration of stars scattered by giant molecular clouds in a galaxy
Stars
Interstellar gas
Short-lived radioactive nuclide 60Fe
Short-lived radioactive nuclide 26Al
Time evolution of the Solar environment in the Galactic disc
Fujimoto, Krumholz, Inutsuka, Boss & Nittler (2020c)
Time evolution of Sun-like motion stars and their local interstellar environments in the Galactic disc for over a hundred million years (see also Fig. 4 in Fujimoto et al. 2020c).
Hydrodynamic simulation of the strongly barred spiral galaxy NGC1300
Fujimoto, Maeda, Habe & Ohta (2020a)
Entire galactic gas disc
Zoomed-in on the bar-end region
Zoomed-in on the bar region
Chemo-hydrodynamic simulation of a normal disc galaxy: Birth environment of the Solar system 4.6 billion years ago
Fujimoto, Krumholz & Tachibana (2018)
Entire galactic disc
Zoomed-in on a spot near the Solar Circle (galactic radius ~ 8 kpc)
Hydrodynamic simulation of a normal disc galaxy: Giant molecular cloud's dynamics
Fujimoto, Chevance, Haydon, Krumholz & Kruijssen (2019)
Entire galactic gas disc
Zoomed-in on a spot near the Solar Circle (Black dots show GMC's locations)
Entire galactic gas disc