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M. Walker

90 papers hereh-index 457.7k citations139 works total

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

author position
  • sole author1
  • first author12
  • middle author47
  • last author23

Across the 83 of 90 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA54
  • astro-ph11
  • astro-ph.CO10
  • astro-ph.SR6
  • astro-ph.HE4
  • astro-ph.IM4
same name
  • M. Walker — 80 papers, h 69
  • M. Walker — 59 papers
  • M. Walker — 55 papers, h 23
  • M. Walker — 29 papers, h 17
  • M. Walker — 27 papers
  • M. Walker — 25 papers, h 22

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
20052023
most citedA Method for Measuring (Slopes of) the Mass Profiles of Dwarf Spheroidal Galaxies

655 citations · 7.9k across the 89 of their papers we have counts for

collaborators
Showing 2019 · astro-ph.GAShow all

2 papers · 2 filters

astro-ph.GA2019★ 9 cited

Dynamical Masses and Mass-to-light Ratios of Resolved Massive Star Clusters. I. NGC 419 and NGC 1846

Ying-Yi Song, Mario Mateo, A. D. Mackey +4

As an introduction of a kinematic survey of Magellanic Cloud (MC) star clusters, we report on the dynamical masses and mass-to-light (M/L) ratios of NGC 419 (SMC) and NGC 1846 (L…

astro-ph.GA2019★ 22 cited

Signatures of Tidal Disruption in Ultra-Faint Dwarf Galaxies: A Combined HST, Gaia, and MMT/Hectochelle Study of Leo V

Burçin Mutlu-Pakdil, David J. Sand, Matthew G. Walker +10

The ultra-faint dwarf galaxy Leo V has shown both photometric overdensities and kinematic members at large radii, along with a tentative kinematic gradient, suggesting that it may…

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