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M. C. Begelman

4 papers here

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.GA1
  • astro-ph.SR1
same name
  • M. C. Begelman — 3 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

collaborators

4 papers

astro-ph.HE2025

Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots

Matteo Cantiello, Jake B. Hassan, Rosalba Perna +5

The JWST discovery of "Little Red Dots" (LRDs) has revealed a population of compact, red sources at z∼5−10 that likely host supermassive black holes (SMBHs). Recent observat…

astro-ph.SR2025

The Growth of the Central Black Holes in Quasi-stars

Jake Hassan, Rosalba Perna, Matteo Cantiello +3

Observations by JWST have confirmed the presence of supermassive black holes (BHs) at redshifts z≳10, lending support to scenarios in which BHs experience rapid growth thro…

astro-ph.GA2025

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.HE2025

Energy Diffusion and Advection Coefficients in Kinetic Simulations of Relativistic Plasma Turbulence

Kai W. Wong, Vladimir Zhdankin, Dmitri A. Uzdensky +2

Turbulent, relativistic nonthermal plasmas are ubiquitous in high-energy astrophysical systems, as inferred from broadband nonthermal emission spectra. The underlying turbulent non…

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