159 citations · 1.4k across the 29 of their papers we have counts for
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PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
Thomas G. Bisbas, Ewine F. van Dishoeck, Chia-Yu Hu +1
Determining the atomic and molecular content of the interstellar medium (ISM) as a function of environmental parameters is of fundamental importance to understand the star-formatio…
Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
Natalia Lahén, Thorsten Naab, Guinevere Kauffmann +6
We present new GRIFFIN project hydrodynamical simulations that model the formation of galactic star cluster populations in low-metallicity () dwarf galaxies, including r…
Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods
Chia-Yu Hu, Matthew C. Smith, Romain Teyssier +8
We present a suite of high-resolution simulations of an isolated dwarf galaxy using four different hydrodynamical codes: {\sc Gizmo}, {\sc Arepo}, {\sc Gadget}, and {\sc Ramses}. A…
The origin of the [CII]-deficit in a simulated dwarf galaxies starburst
Thomas G. Bisbas, Stefanie Walch, Thorsten Naab +6
We present [CII] synthetic observations of smoothed particle hydrodynamics (SPH) simulations of a dwarf galaxy merger. The merging process varies the star-formation rate by more th…
Dependence of on metallicity, intensity, and spatial scale in a self-regulated interstellar medium
Chia-Yu Hu, Andreas Schruba, Amiel Sternberg +1
We study the CO(1-0)-to-H conversion factor () and the line ratio of CO(2-1)-to-CO(1-0) () across a wide range of metallicity ()…