Galactic emissions: seeing through the Galaxy |
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Affiliation: | 1. CESR, 9, avenue du Colonel Roche, BP 4346, 31028 Toulouse cedex 04, France;2. IAS, bâtiment 121, campus d''Orsay, 91405 Orsay cedex, France |
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Abstract: | The diffuse matter in our Galaxy is certainly to be damned by the cosmologist because it pollutes the CMB sky with the various emissions from its components: dust, ionised gas (free–free) and energetic particles (synchrotron). We detail here our knowledge, but also the unknowns, regarding these radiation sources. As we are not in a position to be able to physically escape our Galaxy, the better knowledge of these foreground components is our only hope to build a consistent model which will at least allow us a virtual escape. However, the detailed understanding of the physics of the different emissions and of the large scale distribution of the various emitters is a delight for many of us. We will show here some aspects, with a peculiar emphasis on a possible emission from tiny rotating grains. To cite this article: M. Giard, G. Lagache, C. R. Physique 4 (2003). |
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