
Supernovae such as G1.9+0.3, at the centre of the Milky Way could be responsible for the unexplained "WMAP haze"
Instead, the signal could be produced by amplified cosmic rays generated when particularly large stars explode, says Peter Biermann of the Max Planck Institute for Radioastronomy in Bonn, Germany, and colleagues.
The centre of our galaxy has a high number of massive stars compared with elsewhere. These stars are surrounded by particularly strong magnetic stellar winds. At the star's polar regions, the wind's magnetic field is parallel to the direction of travel of any escaping cosmic rays kicked out by the supernova. This configuration - plus the particularly high turbulence in the galactic centre caused by the high concentration of stars - may be increasing the energy of the cosmic rays, says the team. They have submitted the paper to The Astrophysical Journal.










