Model tests show that the far-IR slope is a degenerate tracer of the silicate-to-carbon ratio, and PRIMA's mid-IR spectra and far-IR polarimetry are forecast to break that degeneracy in M31.
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The radial variation of the silicate-to-carbon ratio in M31 probed by PRIMA
Model tests show that the far-IR slope is a degenerate tracer of the silicate-to-carbon ratio, and PRIMA's mid-IR spectra and far-IR polarimetry are forecast to break that degeneracy in M31.