263 citations · 702 across the 4 of their papers we have counts for
5 papers
A fundamental test for stellar feedback recipes in galaxy simulations
Yusuke Fujimoto, Mélanie Chevance, Daniel T. Haydon +2
Direct comparisons between galaxy simulations and observations that both reach scales < 100 pc are strong tools to investigate the cloud-scale physics of star formation and feedbac…
Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
J. M. Diederik Kruijssen, Andreas Schruba, Mélanie Chevance +7
The physics of star formation and the deposition of mass, momentum, and energy into the interstellar medium by massive stars (`feedback') are the main uncertainties in modern cosmo…
Cloud Scale ISM Structure and Star Formation in M51
Adam K. Leroy, Eva Schinnerer, Annie Hughes +17
We compare the structure of molecular gas at pc resolution to the ability of gas to form stars across the disk of the spiral galaxy M51. We break the PAWS survey into pc…
A milestone toward understanding PDR properties in the extreme environment of LMC-30Dor
M. Chevance, S. C. Madden, V. Lebouteiller +11
More complete knowledge of galaxy evolution requires understanding the process of star formation and interaction between the interstellar radiation field and the interstellar mediu…
The Herschel Dwarf Galaxy Survey: I. Properties of the low-metallicity ISM from PACS spectroscopy
D. Cormier, S. C. Madden, V. Lebouteiller +17
The far-infrared (FIR) lines are key tracers of the physical conditions of the interstellar medium (ISM) and are becoming workhorse diagnostics for galaxies throughout the universe…