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M. C. Begelman

21 papers hereh-index 101.3k citations19 works total

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

author position
  • first author2
  • middle author7
  • last author11

Across the 20 of 21 papers where every author was matched, so the position is known.

fields
  • astro-ph9
  • astro-ph.HE6
  • astro-ph.GA4
  • astro-ph.CO1
  • astro-ph.SR1
same name
  • M. C. Begelman — 8 papers, h 3

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
19972026
most citedHydrodynamical Non-radiative Accretion Flows in Two-Dimensions

390 citations · 1.5k across the 20 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

4 papers · 1 filter

astro-ph.GA2026

Constraints on the Gas Geometry Surrounding Little Red Dots through Narrow-Line Diagnostics

Visal Sok, Erica J. Nelson, Mitchell C. Begelman +10

Little Red Dots (LRDs) are a recently identified population of high-redshift sources, with a common interpretation being accreting black holes embedded within a spherical, opticall…

astro-ph.GA2025★ 27 cited

Little Red Dots As Late-stage Quasi-stars

Mitchell C. Begelman, Jason Dexter

We argue that the "Little Red Dots" (LRDs) discovered with the James Webb Space Telescope are quasi-stars in their late stages of evolution. Quasi-stars are hypothetical objects pr…

astro-ph.GA2024

Quasi-stars as a Means of Rapid Black Hole Growth in the Early Universe

Eric R. Coughlin, Mitchell C. Begelman

JWST observations demonstrate that supermassive black holes (SMBHs) exist by redshifts z≳10, providing further evidence for "direct collapse" black hole (BH) formation, w…

astro-ph.GA2024

Which came first: supermassive black holes or galaxies? Insights from JWST

Joseph Silk, Mitchell Begelman, Colin Norman +2

Insights from JWST observations suggest that AGN feedback evolved from a short-lived, high redshift phase in which radiatively cooled turbulence and/or momentum-conserving outflows…

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