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researcher

J. Butterworth

4 papers hereh-index 679 citations15 works total

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

author position
  • first author2
  • middle author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
same name
  • J. Butterworth — 143 papers, h 33
  • J. Butterworth — 48 papers, h 103
  • J. Butterworth — 4 papers, h 8
  • J. Butterworth — 1 paper, h 6
  • J. Butterworth — 1 paper, h 68
  • J. Butterworth — 1 paper, h 52

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.GA2025

A multi-scale investigation into the diagnostic potential of the HCN/HCO+ ratio for AGN and starburst activity in nearby galaxies

J. Butterworth, S. Viti, Y. Wang

(Abridged) The identification of AGN and SB regions in galaxies is crucial for understanding the role of various physical processes in galaxy evolution. Molecular line ratios, such…

astro-ph.GA2024

First detection of a deuterated molecule in a starburst environment within NGC 253

J. Butterworth, S. Martín, V. M. Rivilla +7

Deuterium was primarily created during the Big Bang Nucleosynthesis (BBN). This fact, alongside its fractionation reactions resulting in enhanced abundances of deuterated molecules…

astro-ph.GA2024

Neural Network Constraints on the Cosmic-Ray Ionization Rate and Other Physical Conditions in NGC 253 with ALCHEMI Measurements of HCN and HNC

Erica Behrens, Jeffrey G. Mangum, Serena Viti +15

We use a neural network model and ALMA observations of HCN and HNC to constrain the physical conditions, most notably the cosmic-ray ionization rate (CRIR, zeta), in the Central Mo…

astro-ph.GA2024

An ALCHEMI inspection of sulphur-bearing species towards the central molecular zone of NGC 253

M. Bouvier, S. Viti, E. Behrens +19

Sulphur-bearing species are detected in various environments within Galactic star-forming regions and are particularly abundant in the gas phase of outflows and shocks, and photo-d…

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