J. Jackson

activity

19982023

most citedThe Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE Data

848 citations · 7.9k across the 67 of their papers we have counts for

collaborators

Showing 2019 · astro-ph.GAShow all

3 papers · 2 filters

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 NH $_{3}$ velocity dispersions ( $σ \sim 8 km s^{- 1}$ ) and bright, narrow NH $_{3}$ (3,3) line…

astro-ph.GA2019★ 207 cited

The ALMA Survey of 70 $μ$ m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

Patricio Sanhueza, Yanett Contreras, Benjamin Wu +20

(Abridged) ASHES has been designed to systematically characterize the earliest stages and to constrain theories of high-mass star formation. A total of 12 massive (>500 $M_{⊙}$ …

astro-ph.GA2019★ 107 cited

'The Brick' is not a brick: A comprehensive study of the structure and dynamics of the Central Molecular Zone cloud G0.253+0.016

J. D. Henshaw, A. Ginsburg, T. J. Haworth +19

In this paper we provide a comprehensive description of the internal dynamics of G0.253+0.016 (a.k.a. 'the Brick'); one of the most massive and dense molecular clouds in the Galaxy…

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

The ALMA Survey of 70 μm dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

'The Brick' is not a brick: A comprehensive study of the structure and dynamics of the Central Molecular Zone cloud G0.253+0.016

The ALMA Survey of 70 $μ$ m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation