GMC Collisions as Triggers of Star Formation. I. Parameter Space Exploration with 2D Simulations
Benjamin Wu (1), Sven Van Loo (2,3), Jonathan C. Tan (1,4), Simon, Bruderer (5) ((1) Department of Physics, University of Florida, (2) School of, Physics, Astronomy, University of Leeds, (3) Harvard-Smithsonian Center, for Astrophysics, (4) Department of Astronomy

TL;DR
This study uses 2D MHD simulations to explore how giant molecular cloud collisions can trigger star formation by increasing clump densities, with specific focus on magnetic effects and observational diagnostics.
Contribution
It introduces a new multiphase ISM model with PDR-based heating/cooling and systematically investigates collision parameters affecting star formation.
Findings
Cloud collisions can increase clump density by 2-3 times.
Magnetic field strength and collision velocity significantly influence collapse.
The ratio of CO emission lines serves as a diagnostic for GMC collisions.
Abstract
We utilize magnetohydrodynamic (MHD) simulations to develop a numerical model for GMC-GMC collisions between nearly magnetically critical clouds. The goal is to determine if, and under what circumstances, cloud collisions can cause pre-existing magnetically subcritical clumps to become supercritical and undergo gravitational collapse. We first develop and implement new photodissociation region (PDR) based heating and cooling functions that span the atomic to molecular transition, creating a multiphase ISM and allowing modeling of non-equilibrium temperature structures. Then in 2D and with ideal MHD, we explore a wide parameter space of magnetic field strength, magnetic field geometry, collision velocity, and impact parameter, and compare isolated versus colliding clouds. We find factors of ~2-3 increase in mean clump density from typical collisions, with strong dependence on collision…
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