478 citations · 4.7k across the 99 of their papers we have counts for
6 papers · 1 filter
Is the molecular KS relationship universal down to low metallicities?
David J. Whitworth, Rowan J. Smith, Robin Tress +4
In recent years it has been speculated that in extreme low metallicity galactic environments, stars form in regions that lack H2. In this paper we investigate how changing the meta…
ALMA observations of the Extended Green Object G19.010.03: I. A Keplerian disc in a massive protostellar system
Gwenllian M. Williams, Claudia J. Cyganowski, Crystal L. Brogan +6
Using the Atacama Large Millimetre/submillimeter Array (ALMA) and the Karl G. Jansky Very Large Array (VLA), we observed the Extended Green Object (EGO) G19.010.03 with sub-arcs…
Dynamically Driven Inflow onto the Galactic Center and its Effect upon Molecular Clouds
H Perry Hatchfield, Mattia C. Sormani, Robin G. Tress +4
The Galactic bar plays a critical role in the evolution of the Milky Way's Central Molecular Zone (CMZ), driving mass inward toward the Galactic Center via gas flows known as dust…
High-resolution CARMA Observation of Molecular Gas in the North America and Pelican Nebulae
Shuo Kong, Héctor G. Arce, John M. Carpenter +15
We present the first results from a CARMA high-resolution CO(1-0), CO(1-0), and CO(1-0) molecular line survey of the North America and Pelican (NAP) Nebulae. C…
The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?
Hideaki Takemura, Fumitaka Nakamura, Shuo Kong +29
Applying dendrogram analysis to the CARMA-NRO CO (=1--0) data having an angular resolution of 8", we identified 692 dense cores in the Orion Nebula Cluster (ONC) r…
SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
Karen Pardos Olsen, Blakesley Burkhart, Mordecai-Mark Mac Low +9
We present an update to the framework called SImulator of GAlaxy Millimeter/submillimeter Emission (SÍGAME). SÍGAME derives line emission in the far-infrared (FIR) for galaxies in…