Radiative filaments in the Cygnus Loop exhibit thermal radio spectra resembling HII regions instead of typical SNR non-thermal emission.
I., Leer E., Skadron G.\ 1977, The acceleration of cosmic-rays by shock waves, International Cosmic Ray Conference, 11:132-137
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The radio emission from radiative filaments of Cygnus Loop
Radiative filaments in the Cygnus Loop exhibit thermal radio spectra resembling HII regions instead of typical SNR non-thermal emission.