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- W1569259280 abstract "Abstract Observations of H92α radio recombination line (RRL) and continuum emission were made towards three Celnik positions of the Rosette Nebula . The electron temperature Te(LTE) was derived for each position giving an average value of 7980±580 K. A non-LTE modelling was made which could describe the dependence of line contrast (TL/TC), Te(LTE) and line width on quantum number (n). The modelling together with a review of available data show that the Rosette Nebula should contain clumps with densities up to ∼103 cm−3. The unexpected VLSR measured at one of the three positions could be interpreted as a possible jet, or some dense compact part (clump) of the HII region, moving toward the observer." @default.
- W1569259280 created "2016-06-24" @default.
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- W1569259280 date "2002-10-01" @default.
- W1569259280 modified "2023-09-26" @default.
- W1569259280 title ": RRL observations of 92α transition and the modelling" @default.
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- W1569259280 doi "https://doi.org/10.1016/s1384-1076(02)00159-8" @default.
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