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Michael J. Williams

10 papers hereh-index 7543 citations17 works total

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

author position
  • first author5
  • last author4

Across the 9 of 10 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA6
  • astro-ph.CO3
  • astro-ph1
same name
  • Michael J. Williams — 7 papers, h 5
  • Michael J. Williams — 3 papers, h 4
  • Michael J. Williams — 3 papers, h 3
  • Michael J. Williams — 3 papers, h 2
  • Michael J. Williams — 2 papers, h 1
  • Michael J. Williams — 1 paper

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
20082014
most citedThe Tully-Fisher relations of early-type spiral and S0 galaxies

204 citations · 586 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

3 papers · 1 filter

astro-ph.CO2012★ 62 cited

Measuring Dark Matter Profiles Non-Parametrically in Dwarf Spheroidals: An Application to Draco

John R. Jardel, Karl Gebhardt, Maximilian Fabricius +2

We introduce a novel implementation of orbit-based (or Schwarzschild) modeling that allows dark matter density profiles to be calculated non-parametrically in nearby galaxies. Our…

astro-ph.CO2012★ 88 cited

Molecular gas in the centre of nearby galaxies from VLT/SINFONI integral field spectroscopy - I. Morphology and mass inventory

X. Mazzalay, R. P. Saglia, Peter Erwin +7

We present the first results of an analysis of the properties of the molecular gas in the nuclear regions (r < 300 pc) of a sample of six nearby galaxies, based on new high spatial…

astro-ph.CO2012★ 20 cited

Secular evolution in action: central values and radial trends in the stellar populations of boxy bulges

Michael J. Williams, Martin Bureau, Harald Kuntschner

We determine central values and radial trends in the stellar populations of the bulges of a sample of 28 edge-on S0-Sb disk galaxies, 22 of which are boxy/peanut-shaped (and theref…

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