Radiative filaments in the Cygnus Loop exhibit thermal radio spectra resembling HII regions instead of typical SNR non-thermal emission.
E., et al., 2019, @doi [ ] 10.1093/mnras/sty3021 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.4617S 482
2 Pith papers cite this work. Polarity classification is still indexing.
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Most dusty early-type galaxies exhibit recent star formation components in their stellar populations, as revealed by spectral fitting of 15 nearby examples with a non-dusty control comparison.
citing papers explorer
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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.
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Stellar Population Characterisations in nearby, dusty Early-Type Galaxies
Most dusty early-type galaxies exhibit recent star formation components in their stellar populations, as revealed by spectral fitting of 15 nearby examples with a non-dusty control comparison.