activity
20182022
most citedAsymmetric Line Profiles in Dense Molecular Clumps Observed in MALT90: Evidence for Global Collapse

35 citations · 109 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2022★ 28 cited

The ALMA Survey of 70 Dark High-mass Clumps in Early Stages (ASHES). VII: Chemistry of Embedded Dense Cores

Shanghuo Li, Patricio Sanhueza, Xing Lu +15

We present a study of chemistry toward 294 dense cores in 12 molecular clumps using the data obtained from the ALMA Survey of 70 dark High-mass clumps in Early Stages (ASH…

astro-ph.GA2022★ 29 cited

The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VI. The core-scale CO-depletion

Giovanni Sabatini, Stefano Bovino, Patricio Sanhueza +11

Studying the physical and chemical properties of cold and dense molecular clouds is crucial for the understanding of how stars form. Under the typical conditions of infrared dark c…

astro-ph.GA2020★ 2 cited

Characterizing [C II] Line Emission In Massive Star Forming Clumps

James M. Jackson, David Allingham, Nicholas Killerby-Smith +7

Because the 157.74 micron [C II] line is the dominant coolant of star-forming regions, it is often used to infer the global star-formation rates of galaxies. By characterizing the…

astro-ph.GA2019★ 10 cited

The Interaction Between the Supernova Remnant W41 and the Filamentary Infrared Dark Cloud G23.33-0.30

Taylor G. Hogge, James M. Jackson, David Allingham +6

G23.33-0.30 is a 600 infrared dark molecular filament that exhibits large NH velocity dispersions () and bright, narrow NH(3,3) line…

astro-ph.GA2018★ 5 cited

G337.342-0.119 (the "Pebble"): A Cold, Dense, High-Mass Molecular Cloud with Unusually Large Linewidths and a Candidate High-Mass Star Cluster Progenitor

James M. Jackson, Yanett Contreras, Jill M. Rathborne +7

Exactly how high-mass star clusters form, especially the young massive clusters (YMCs: age Myr; mass solar masses), remains an open problem, largely because they are…

astro-ph.GA2018★ 35 cited

Asymmetric Line Profiles in Dense Molecular Clumps Observed in MALT90: Evidence for Global Collapse

James M. Jackson, J. Scott Whitaker, J. M. Rathborne +6

Using molecular line data from the Millimetre Astronomy Legacy Team 90 GHz Survey (MALT90), we have searched the optically thick \hcop\, line for the "blue asymmetry" spectroscopic…