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• W1675364023 abstract "The structure of helium-rich very cool white dwarf atmospheres is investigated if the opacity in the visible and infrared region of the spectrum is mainly due to diatomic and polyatomic species of carbon and hydrogen.molecules. For various abundance ratios of H/He, C/He, 0/He and N/He the gradients of C3, C2H and C2H2 in the outer layers of model atmospheres with T eff ≤ 5000K, log g =8.0 have been computed as well as fluxes for comparison with observed spectra. It is shown that even a reduced oxygen abundance is far from negligible for the overall run of partial pressures." @default.
• W1675364023 created "2016-06-24" @default.
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• W1675364023 date "1997-01-01" @default.
• W1675364023 modified "2023-09-27" @default.
• W1675364023 title "Polyatomic Carbon Molecules in Very Cool Helium-Rich White Dwarfs" @default.
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• W1675364023 doi "https://doi.org/10.1007/978-94-011-5542-7_27" @default.
• W1675364023 hasPublicationYear "1997" @default.
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