4 citations · 4 across the 2 of their papers we have counts for
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astro-ph.GA2025
The Young Ages of 70 μm-dark Clumps Inferred from Carbon Chain Chemistry
Kadin Worthen, Brian E. Svoboda, David S. Meier +4
The physical conditions of the earliest environment of high-mass star formation are currently poorly understood. To that end, we present observations of the carbon chain molecules…
astro-ph.GA2024★ 4 cited
Turbulent Pressure Heats Gas and Suppresses Star Formation in Galactic Bar Molecular Clouds
Andy Nilipour, Juergen Ott, David S. Meier +6
The Central Molecular Zone (CMZ) of the Milky Way is fed by gas inflows from the Galactic disk along almost radial trajectories aligned with the major axis of the Galactic bar. How…