Speaker
Maxim Pshirkov
(SAI Moscow State University)
Description
Theories of galaxy formation predict the existence of extended gas halo around spiral galaxies. If there are 10-100 nG magnetic fields at several ten kpc distances from the galaxies, extended galactic cosmic ray (CR) haloes could also exist. Galactic CRs could interact with the tenuous hot halo gas to produce observable $\gamma$-rays. In this paper we have performed search for such a halo around the M31 galaxy -- the closest large spiral galaxy. Our analysis of 5.5 years of the Fermi LAT data revealed the presence of a spatially extended emission excess around M31. The data can be fitted using the simplest morphology of a uniformly bright circle. The best fit gave a 4.4$\sigma$ significance for a $3^{\circ}$ (40 kpc) halo with photon flux of $\sim (1.9\pm1.1)\times 10^{-9} ~\mathrm{cm^{-2}s^{-1}}$ and luminosity $(8.4\pm4.6)\times 10^{38} ~\mathrm{erg~s^{-1}}$ in the energy range 0.3--100 GeV. The presence of such a halo compellingly shows that a 10-100 nG magnetic field should extend around M31 up to
a 40 kpc distance.
| Registration number following "ICRC2015-I/" | 798 |
|---|---|
| Collaboration | -- not specified -- |
Author
Maxim Pshirkov
(SAI Moscow State University)
Co-authors
Prof.
Konstantin Postnov
(SAI Moscow State University)
Valery Vasiliev
(MPIA Heidelberg)
