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Journal article

Fingerprints of Galactic Loop I on the Cosmic Microwave Background

Abstract:
We investigate possible imprints of galactic foreground structures such as the "radio loops" in the derived maps of the cosmic microwave background. Surprisingly there is evidence for these not only at radio frequencies through their synchrotron radiation, but also at microwave frequencies where emission by dust dominates. This suggests the mechanism is magnetic dipole radiation from dust grains enriched by metallic iron or ferrimagnetic materials. This new foreground we have identified is present at high galactic latitudes, and potentially dominates over the expected $B$-mode polarization signal due to primordial gravitational waves from inflation.
Publication status:
Published
Peer review status:
Peer reviewed

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Files:
Publisher copy:
10.1088/2041-8205/789/2/L29

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author


Journal:
Astrophysical Journal Letters More from this journal
Volume:
789
Issue:
2
Pages:
L29-L29
Publication date:
2014-01-01
DOI:
EISSN:
2041-8213
ISSN:
2041-8205


Keywords:
Pubs id:
pubs:459636
UUID:
uuid:bb72d876-102b-43d7-930e-5251903d13eb
Local pid:
pubs:459636
Source identifiers:
459636
Deposit date:
2014-05-18

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