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- W3099836273 endingPage "103" @default.
- W3099836273 startingPage "103" @default.
- W3099836273 abstract "The Small Magellanic Cloud (SMC) has surprisingly strong submm and mm-wavelength emission that is inconsistent with standard dust models, including those with emission from spinning dust. Here we show that the emission from the SMC may be understood if the interstellar dust mixture includes magnetic nanoparticles, emitting magnetic dipole radiation resulting from thermal fluctuations in the magnetization. The magnetic grains can be metallic iron, magnetite Fe3O4, or maghemite gamma-Fe2O3. The required mass of iron is consistent with elemental abundance constraints. The magnetic dipole emission is predicted to be polarized orthogonally to the normal electric dipole radiation if the nanoparticles are inclusions in larger grains. We speculate that other low-metallicity galaxies may also have a large fraction of the interstellar Fe in magnetic materials." @default.
- W3099836273 created "2020-11-23" @default.
- W3099836273 creator A5023974267 @default.
- W3099836273 creator A5045810979 @default.
- W3099836273 date "2012-09-06" @default.
- W3099836273 modified "2023-09-25" @default.
- W3099836273 title "THE SUBMILLIMETER AND MILLIMETER EXCESS OF THE SMALL MAGELLANIC CLOUD: MAGNETIC DIPOLE EMISSION FROM MAGNETIC NANOPARTICLES?" @default.
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- W3099836273 doi "https://doi.org/10.1088/0004-637x/757/1/103" @default.
- W3099836273 hasPublicationYear "2012" @default.
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