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researcher

D. Allingham

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author1
  • last author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3

identity via Semantic Scholar / OpenAlex

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

10 citations · 10 across the 1 of their papers we have counts for

collaborators

3 papers

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 M⊙​ infrared dark molecular filament that exhibits large NH3​ velocity dispersions (σ∼8 km s−1) and bright, narrow NH3​(3,3) line…

astro-ph.GA2018

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 <100 Myr; mass >104 solar masses), remains an open problem, largely because they are…

astro-ph.GA2018

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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.