2 papers
astro-ph.HE2025
Polarization properties of synchrotron sources from simulations of relativistic magnetohydrodynamic turbulence
Luca Del Zanna, Niccolò Bucciantini, Simone Landi
The emission from the relativistically hot plasmas of high-energy astrophysical synchrotron sources, pulsar wind nebulae (PWNe) in particular, depends on the level of magnetic fluc…
astro-ph.HE2025
Contribution of young massive star clusters to Galactic diffuse -ray emission
Stefano Menchiari, Giovanni Morlino, Elena Amato +3
Context: Young massive stellar clusters (YMSCs) have emerged as potential -ray sources, after the recent association of a dozen YMSCs with extended -ray emission. The large…