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researcher

N. Killerby-Smith

3 papers hereh-index 212 citations9 works total

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph.GA3

identity via Semantic Scholar / OpenAlex

activity
20192021
most citedThe Interaction Between the Supernova Remnant W41 and the Filamentary Infrared Dark Cloud G23.33-0.30

10 citations · 10 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2021

The MACH HI absorption survey I: Physical conditions of cold atomic gas outside of the Galactic plane

Claire E. Murray, Snežana Stanimirović, Carl Heiles +5

Tracing the transition between the diffuse atomic interstellar medium (ISM) and cold, dense gas is crucial for deciphering the star formation cycle in galaxies. Here we present MAC…

astro-ph.GA2020

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

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