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On the Mechanism of Accretion by Stars

Hermann Bondi, +1 more
- 01 Oct 1944 - 
- Vol. 104, Iss: 5, pp 273-282
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1944-10-01 and is currently open access. It has received 1476 citations till now. The article focuses on the topics: Bondi accretion & Accretion (astrophysics).

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Modelling feedback from stars and black holes in galaxy mergers

TL;DR: In this paper, a coarse-grained representation of the properties of the interstellar medium (ISM) and BH accretion starting from basic physical assumptions is proposed to incorporate feedback from star formation and black hole accretion into simulations of isolated and merging galaxies.
Journal ArticleDOI

Modeling feedback from stars and black holes in galaxy mergers

TL;DR: In this paper, a coarse-grained representation of the properties of the interstellar medium and black hole accretion starting from basic physical assumptions is proposed, and the impact of these effects can be included on resolved scales.
Journal ArticleDOI

A Unified, Merger-driven Model of the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes, and Galaxy Spheroids

TL;DR: In this article, an evolutionary model for starbursts, quasars, and spheroidal galaxies is presented, in which mergers between gas-rich galaxies drive nuclear inflows of gas, producing starburst and feeding the buried growth of supermassive black holes (BHs) until feedback expels gas and renders a briefly visible optical quasar.
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Evolution of binary stars and the effect of tides on binary populations

TL;DR: In this paper, a rapid binary-evolution algorithm was proposed to model the formation and evolution of binary systems, including all aspects of single-star evolution, features such as mass transfer, mass accretion, common envelope evolution, collisions, supernova kicks and angular momentum loss mechanisms.
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