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- W2043891202 abstract "The typical extinction curve for the Small Magellanic Cloud (SMC), in contrast to that for the Galaxy, has no bump at 2175 Å and a steeper rise into the far-ultraviolet. For the Galaxy, the interpretation of the extinction, and therefore the dust content of the interstellar medium, has been greatly assisted by measurements of the wavelength dependence of the polarization. Up to the present, no such measurements existed for the SMC." @default.
- W2043891202 created "2016-06-24" @default.
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- W2043891202 date "1997-08-20" @default.
- W2043891202 modified "2023-10-05" @default.
- W2043891202 title "Dust in the Small Magellanic Cloud: Interstellar Polarization and Extinction" @default.
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- W2043891202 doi "https://doi.org/10.1086/304434" @default.
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