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Bondi on spherically symmetric accretion

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arxiv 2004.00203 v1 pith:OFGCCOBR submitted 2020-04-01 astro-ph.HE astro-ph.GA

classification astro-ph.HEastro-ph.GA
keywords accretionbondiastrophysicsformationsphericallyacrossalthoughanalysis
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Hermann Bondi's 1952 paper "On spherically symmetrical accretion" is recognized as one of the foundations of accretion theory. Although Bondi later remarked that it was "not much more than an examination exercise", his mathematical analysis of spherical accretion on to a point mass has found broad use across fields of astrophysics that were embryonic or non-existent at the time of the paper's publication. In this non-technical review, I describe the motivations for Bondi's work, and briefly discuss some of the applications of Bondi accretion in high energy astrophysics, galaxy formation, and star formation.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Dynamics, Ringdown, and Accretion-Driven Multiple Quasi-Periodic Oscillations of Kerr-Bertotti-Robinson Black Holes

    gr-qc 2026-02 conditional novelty 5.0 of 10

    Simulations of Bondi-Hoyle-Lyttleton accretion onto a Kerr-Bertotti-Robinson black hole produce alternating flip-flop shock and torus states whose power-spectral peaks resemble the low- and high-frequency QPOs seen in...

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