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• W4378506189 abstract "During the commissioning of {em JWST}, the Medium-Resolution Spectrometer (MRS) on the Mid-Infrared Instrument (MIRI) observed the planetary nebula SMP LMC 058 in the Large Magellanic Cloud. The MRS was designed to provide medium resolution (R = $lambda$/$Deltalambda$) 3D spectroscopy in the whole MIRI range. SMP LMC 058 is the only source observed in {em JWST} commissioning that is both spatially and spectrally unresolved by the MRS and is a good test of {em JWST's} capabilities. The new MRS spectra reveal a wealth of emission lines not previously detected in this planetary nebula. From these lines, the spectral resolving power ($lambda$/$Deltalambda$) of the MRS is confirmed to be in the range R $=$ 4000 to 1500, depending on the MRS spectral sub-band. In addition, the spectra confirm that the carbon-rich dust emission is from SiC grains and that there is little to no time evolution of the SiC dust and emission line strengths over a 17-year epoch. These commissioning data reveal the great potential of the MIRI MRS for the study of circumstellar and interstellar material." @default.
• W4378506189 created "2023-05-27" @default.
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• W4378506189 date "2023-01-30" @default.
• W4378506189 modified "2023-10-01" @default.
• W4378506189 title "Observations of the Planetary Nebula SMP LMC 058 with the JWST MIRI Medium Resolution Spectrometer" @default.
• W4378506189 doi "https://doi.org/10.48550/arxiv.2301.13233" @default.
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