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Michael Williams

2 papers hereh-index 12 citations3 works total

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

author position
  • middle author2

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

fields
  • astro-ph.HE2
same name
  • Michael Williams — 2 papers
  • Michael Williams — 2 papers, h 2
  • Michael Williams — 2 papers, h 3
  • Michael Williams — 1 paper, h 7
  • Michael Williams — 1 paper, h 4

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

most citedCharacteristics of Powerful Radio Galaxies

2 citations · 2 across the 1 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2025

How a Klein-Nishina Modified Eddington limited accretion explains rapid black hole growth in the early universe

Jackson Frangos, Erick Rosen, Michael Williams +2

The discovery of quasars and their supermassive black holes (SMBHs) over 109M⊙​ merely hundreds of millions of years after the Big Bang generates tension with the idea…

astro-ph.HE2024★ 2 cited

Characteristics of Powerful Radio Galaxies

Chandra B. Singh, Michael Williams, David Garofalo +3

Mature radio galaxies such as M87 belong to a specific subclass of active galaxies (AGN) whose evolution in time endows them with five distinguishing characteristics, including (1)…

astro-ph.HE2024

The properties of FR0 radio galaxies as intermediate objects in the evolution of radio galaxies

David Garofalo, Chandra B. Singh, Eddie Harmon +2

The counter-rotation between black holes and accretion disk configuration was introduced over a decade ago to elucidate the nature of the radio loud/radio-quiet dichotomy and the j…

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