Dust from refractory r-process elements forms efficiently in kilonova ejecta and explains the observed late-time infrared spectra.
J., Espenak, F., Jennings, D
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Magnetoacoustic cutoff frequency rises with height from 3.0 mHz at 0.38 Mm to 8.5 mHz at 1.2 Mm based on cross-wavelet analysis of IRIS Doppler velocities.
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Heavy element dust explains the late-time spectra of kilonovae
Dust from refractory r-process elements forms efficiently in kilonova ejecta and explains the observed late-time infrared spectra.
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Height Variations of Magnetoacoustic Cutoff Frequency in the Solar Atmosphere
Magnetoacoustic cutoff frequency rises with height from 3.0 mHz at 0.38 Mm to 8.5 mHz at 1.2 Mm based on cross-wavelet analysis of IRIS Doppler velocities.