| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1770864 | Astroparticle Physics | 2012 | 7 Pages |
Abstract
⺠We present 3D models of the Galactic magnetic field including regular and turbulent components. ⺠We compute the expected dust and synchrotron emission. ⺠We compare expectations to the WMAP and Archeops data. ⺠We propose a consistent model of the Galaxy in the frequency range from 33 to 353 GHz. ⺠Model useful for CMB studies.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
L. Fauvet, J.F. MacÃas-Pérez, F.X. Désert,