Super-Serkowski UV polarization excesses are explained by enhanced RAT alignment under B-star EUV radiation (plus DG at the shortest wavelengths), while Serkowski curves are reproduced by RAT alone in cold neutral medium conditions.
Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy’s Evolution (sage)
2 Pith papers cite this work. Polarity classification is still indexing.
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The paper reviews dust production, destruction and growth processes in galaxies, compiles literature data on comoving dust mass density, presents evidence for and against interstellar dust growth, and identifies the high-redshift dust budget as needing further study.
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Grain Alignment and Dust Evolution Physics with Polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra
Super-Serkowski UV polarization excesses are explained by enhanced RAT alignment under B-star EUV radiation (plus DG at the shortest wavelengths), while Serkowski curves are reproduced by RAT alone in cold neutral medium conditions.
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Interstellar dust production, destruction and effects of dust depletion in galaxies
The paper reviews dust production, destruction and growth processes in galaxies, compiles literature data on comoving dust mass density, presents evidence for and against interstellar dust growth, and identifies the high-redshift dust budget as needing further study.