T. Hogge

activity

20182025

most citedThe chemical structure of young high-mass star-forming clumps: (II) parsec-scale CO depletion and deuterium fraction of

HC O^{+}

29 citations · 84 across the 6 of their papers we have counts for

collaborators

Showing 2019Show all

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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…