Polarized Foreground from Thermal Dust Emission

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dc.creatorPrunet, S.
dc.creatorLazarian, A.
dc.date1999-02-22
dc.date.accessioned2026-07-07T02:30:34Z
dc.date.available2026-07-07T02:30:34Z
dc.descriptionIn this review, we intend to present the current knowledge of the polarized emission from thermal dust in our Galaxy. We show different methods to estimate the spatial distribution statistics of this emission in the lack of any data from the diffuse ISM, and compare it to the expected CMB polarized signal. We finally show how this contaminant could be efficiently removed from CMB maps using multi-frequency observations.
dc.description21 pages, 9 figures, Review for the Sloan Summit on Foregrounds
dc.identifierhttps://arxiv.org/abs/astro-ph/9902314
dc.identifierhttp://arxiv.org/abs/astro-ph/9902314
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13855
dc.subjectAstrophysics
dc.titlePolarized Foreground from Thermal Dust Emission
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