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M. T. Hogan

3 papers here

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

author position
  • first author1
  • middle author1

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

fields
  • astro-ph.GA2
  • astro-ph.HE1
ORCID 0000-0002-7031-721X

identity via Semantic Scholar / OpenAlex

most citedMolecular Gas Along a Bright H-alpha Filament in 2A 0335+096 Revealed by ALMA

53 citations · 143 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2016★ 46 cited

Mass Distribution in Galaxy Cluster Cores

M. T. Hogan, B. R. McNamara, F. Pulido +5

Many processes within galaxy clusters, such as those believed to govern the onset of thermally unstable cooling and AGN feedback, are dependent upon local dynamical timescales. How…

astro-ph.GA2016★ 53 cited

Molecular Gas Along a Bright H-alpha Filament in 2A 0335+096 Revealed by ALMA

A. N. Vantyghem, B. R. McNamara, H. R. Russell +17

We present ALMA CO(1-0) and CO(3-2) observations of the brightest cluster galaxy (BCG) in the 2A 0335+096 galaxy cluster (z = 0.0346). The total molecular gas mass of (1.13+/-0.15)…

astro-ph.HE2014★ 44 cited

A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades

K. L. Dutson, A. C. Edge, J. A. Hinton +3

Emission from the active nucleus in the core of the brightest cluster galaxy of the Perseus cluster, NGC 1275, has varied dramatically over the past four decades. Prompted by the F…

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