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Cited by 2,526

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Accretion Power in Astrophysics

Frank, Juhan, King, Andrew, Raine, Derek·2002·Cambridge University Press eBooks
DOI 10.1017/cbo9781139164245
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Abstract

Accretion Power in Astrophysics examines accretion as a source of energy in both binary star systems containing compact objects, and in active galactic nuclei. Assuming a basic knowledge of physics, the authors describe the physical processes at work in accretion discs and other accretion flows. The first three chapters explain why accretion is a source of energy, and then present the gas dynamics and plasma concepts necessary for astrophysical applications. The next three chapters then develop accretion in stellar systems, including accretion onto compact objects. Further chapters give extensive treatment of accretion in active galactic nuclei, and describe thick accretion discs. A new chapter discusses recently discovered accretion flow solutions. The third edition is greatly expanded and thoroughly updated. New material includes a detailed treatment of disc instabilities, irradiated discs, disc warping, and general accretion flows. The treatment is suitable for advanced undergraduates, graduate students and researchers.

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Metadata

Authors
Frank, J., King, A., & Raine, D.
Venue
Cambridge University Press eBooks
Publisher
Cambridge University Press
Published
2002-01-17
DOI
10.1017/cbo9781139164245
OpenAlex
W2985443361
Cited by
2,526
References
0
FWCI
57.39
Type
book
Language
en
Open access
closed

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CoChat. (2026). Citation check: Accretion Power in Astrophysics. https://app.cochat.ai/papers/10.1017/cbo9781139164245
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Frank, J., King, A., & Raine, D. (2002). Accretion Power in Astrophysics. Cambridge University Press eBooks. https://doi.org/10.1017/cbo9781139164245

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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.