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• W2120900521 abstract "We demonstrate that the observed increase of some nebular line ratios with height above the midplane in the diffuse ionized gas (DIG) in the Milky Way and other galaxies is a natural consequence of the progressive hardening of the radiation field far from the midplane ionizing sources. To obtain increasing temperatures and line ratios away from the midplane, our photoionization simulations of a multicomponent interstellar medium do not require as much additional heating (over and above that from photoionization) as previous studies that employed one‐dimensional, spherically averaged models." @default.
• W2120900521 created "2016-06-24" @default.
• W2120900521 creator A5020379510 @default.
• W2120900521 creator A5077947407 @default.
• W2120900521 date "2004-10-01" @default.
• W2120900521 modified "2023-10-17" @default.
• W2120900521 title "Monte Carlo photoionization simulations of diffuse ionized gas" @default.
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• W2120900521 doi "https://doi.org/10.1111/j.1365-2966.2004.07846.x" @default.
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