Diffuse microwave emission of the interstellar medium : intensity and polarization

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dc.creatorMiville-Deschenes, Marc-Antoine
dc.date2009-05-19
dc.date.accessioned2026-07-07T13:16:29Z
dc.date.available2026-07-07T13:16:29Z
dc.descriptionWith the increasing number of experiments dedicated to the observation of the Cosmic Microwave Background, interest on the detailed properties of the foreground Galactic emission has risen. In particular the focus is shifting towards polarized microwave emission with the goal of detecting signature from primordial gravitational waves and inflation. This review describes the Galactic polarized and unpolarized emissions in the microwave range : free-free, synchrotron, thermal dust and anomalous emission.
dc.descriptionto appear in the ASP proceedings of the Astronomical Polarimetry 2008 conference
dc.identifierhttps://arxiv.org/abs/0905.3094
dc.identifierhttp://arxiv.org/abs/0905.3094
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/230806
dc.subjectAstrophysics of Galaxies
dc.subjectCosmology and Nongalactic Astrophysics
dc.titleDiffuse microwave emission of the interstellar medium : intensity and polarization
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