NenuFAR's 10 to 85 MHz observations of Cas A and Cyg A yield new, higher-resolution constraints on the electron temperature and density of four diffuse interstellar clouds, with T_e about 50% lower and n_e about 35% lower than LOFAR-based estimates.
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Observations of Carbon Radio Recombination Lines with the NenuFAR telescope. I. Cassiopeia A and Cygnus A
NenuFAR's 10 to 85 MHz observations of Cas A and Cyg A yield new, higher-resolution constraints on the electron temperature and density of four diffuse interstellar clouds, with T_e about 50% lower and n_e about 35% lower than LOFAR-based estimates.