EPJ Web Conf.
Volume 125, 2016The 19th International Seminar on High Energy Physics (QUARKS-2016)
|Number of page(s)||3|
|Section||3. Neutrino physics; cosmic rays, astrophysics, cosmology as related to particle physics|
|Published online||28 October 2016|
The Spatial Structure of the WMAP/Planck Haze
1 Institute for Nuclear Research, Russian Academy of Sciences, 117312, Moscow, Russia
2 Faculty of Physics, Lomonosov Moscow State University, 119991, Moscow, Russia
* e-mail: email@example.com
Published online: 28 October 2016
It was recently proposed that the two phenomena, WMAP/Planck haze and Fermi bubbles may have a common origin. In the present paper we analyze the spatial structure of the haze using the Planck 2015 data. It is found that the spatial dimensions and locations of WMAP/Planck haze and Fermi bubbles are compatible within experimental uncertainties for symmetric approximation case, and WMAP/Planck haze appear to be more flattened in galactic latitude direction for the asymmetric approximation case. WMAP/Planck haze possesses north-south asymmetry, it is more intensive in the northern hemisphere. No substructures similar to Fermi bubbles cocoon are identified in Planck data.
© The Authors, published by EDP Sciences, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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