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• W3102808081 abstract "We have imaged the H92α (8.3 GHz), H75α (15 GHz), and H166α (1.4 GHz) Radio Recombination Lines (RRLs) from NGC 253 at resolutions of 4.5 pc (0.4″) , 2.5 pc (0.2″) and 53 pc (4.5″) respectively. The H92α line arises from individual compact sources, most of which possess radio continuum counterparts. The line widths range from ~200 km s-1 for the sources near the radio nucleus to 70–100 km s-1 for the extranuclear ones. These lines are emitted by gas at a density ~104 cm-3. The remainder of the cm-wave RRLs arise in lower density gas (~500 cm-3) with a higher area filling factor and with ten times higher mass. A third component of higher density gas (>104 cm-3) is required to explain the mm-wave RRLs." @default.
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• W3102808081 date "2005-02-22" @default.
• W3102808081 modified "2023-09-23" @default.
• W3102808081 title "Multi-density model of the ionised gas in NGC 253 using radio recombination lines" @default.
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• W3102808081 doi "https://doi.org/10.1051/0004-6361:20041488" @default.
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