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• W2104388200 abstract "Context.A photoionized gas in thermal equilibrium can display a thermal instability, with three or more solutions in the multi-branch region of the S-shape curve that gives the temperature versus the radiation-to-gas-pressure ratio. Many studies have been devoted to this curve and to its dependence on different parameters, always in the optically thin case." @default.
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• W2104388200 date "2007-01-02" @default.
• W2104388200 modified "2023-10-11" @default.
• W2104388200 title "Thermal instability in X-ray photoionized media in active galactic nuclei:" @default.
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• W2104388200 doi "https://doi.org/10.1051/0004-6361:20066089" @default.
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