Modelling the behaviour of accretion flows in X-ray binaries

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Done, Chris, et al. “Modelling the Behaviour of Accretion Flows in X-Ray Binaries”. The Astronomy and Astrophysics Review, vol. 15, no. 1, 2007, pp. 1-66, https://doi.org/10.1007/s00159-007-0006-1.
Done, C., Gierliński, M., & Kubota, A. (2007). Modelling the behaviour of accretion flows in X-ray binaries. The Astronomy and Astrophysics Review, 15(1), 1-66. https://doi.org/10.1007/s00159-007-0006-1
Done C, Gierliński M, Kubota A. Modelling the behaviour of accretion flows in X-ray binaries. The Astronomy and Astrophysics Review. 2007;15(1):1-66.
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The first research to cite this article was titled GRS 1915+105: high-energy insights with SPI/INTEGRAL and was published in 2008. The most recent citation comes from a 2024 study titled GRS 1915+105: high-energy insights with SPI/INTEGRAL . This article reached its peak citation in 2023 , with 87 citations.It has been cited in 48 different journals, 20% of which are open access. Among related journals, the Monthly Notices of the Royal Astronomical Society cited this research the most, with 381 citations. The chart below illustrates the annual citation trends for this article.
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