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M. McDonald

12 papers hereh-index 362 citations12 works total

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

author position
  • first author1
  • middle author9
  • last author1

Across the 11 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA9
  • astro-ph.CO2
  • astro-ph.HE1
same name
  • M. McDonald — 120 papers, h 38
  • M. McDonald — 33 papers, h 17
  • M. McDonald — 15 papers, h 11
  • M. McDonald — 11 papers, h 11
  • M. McDonald — 10 papers, h 10
  • M. McDonald — 8 papers, h 2

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

activity
20142026
most citedRevealing the velocity structure of the filamentary nebula in NGC 1275 in its entirety

60 citations · 123 across the 12 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.GA2026

High-spectral-resolution Observations of the [S II] Emission-line Doublet in the Filamentary Nebula Surrounding NGC 1275

Benjamin Vigneron, Julie Hlavacek-Larrondo, Carter Lee Rhea +10

We analyze new high-spectral resolution SITELLE observations (R = λ/Δλ = 7000) of the filamentary nebula surrounding NGC 1275, central galaxy of the Perseus cluster. We present h…

astro-ph.GA2026

A Kiloparsec-Scale Stellar Cavity in the Center of Abell402-BCG May be Caused by Dynamic Interactions with an Ultramassive Black Hole

Michael McDonald, Gourav Khullar, David Lagattuta +18

We present new observations from JWST NIRCam that reveal a striking kpc-wide cavity in the stellar distribution of the central galaxy in the cluster Abell402. Supporting data from…

astro-ph.CO2026

The Cluster Evolutionary Reference Ensemble at Low-z (CEREAL) Sample of Galaxy Clusters I: X-ray Morphological Properties and Demographics

Laurel White, Michael McDonald, Steven W. Allen +8

With rapid improvements in the assembly of large samples of galaxy clusters, we are approaching the ability to study clusters at z≳2. Evolutionary studies comparing these d…

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