102 citations · 1.2k across the 47 of their papers we have counts for
47 papers
Synchrotron polarization with a partially random magnetic field: general approach, and application to X-ray polarization from SNRs
Rino Bandiera, Oleh Petruk
Diagnostics based on the polarization properties of the synchrotron emission can provide precious information on both the ordered structure and the random level of the magnetic fie…
The nature of the X-ray filaments around bow shock pulsar wind nebulae
Barbara Olmi, Elena Amato, Rino Bandiera +1
Context. We propose that the X-ray filaments emerging from selected bow shock pulsar wind nebulae are due to a charge-separated outflow of electrons and/or positrons escaping the n…
Reverberation of pulsar wind nebulae (III): Modelling of the plasma interface empowering a long term radiative evolution
R. Bandiera, N. Bucciantini, B. Olmi +1
The vast majority of Pulsar Wind Nebulae (PWNe) present in the Galaxy is formed by middle-aged systems characterized by a strong interaction of the PWN itself with the supernova re…
Reverberation of pulsar wind nebulae (II): Anatomy of the "thin-shell'' evolution
R. Bandiera, N. Bucciantini, J. Martín +2
During its early evolution, a pulsar wind nebula (PWN) sweeps the inner part of the supernova ejecta and forms a thin massive shell. Later on, when the shell has been reached by th…
Modeling the γ-ray Pulsar Wind Nebulae population in our Galaxy
M. Fiori, B. Olmi, E. Amato +4
Pulsar wind nebulae (PWNe) represent the largest class of sources that upcoming γ-ray surveys will detect. Therefore, accurate modelling of their global emission properties is one…
Revisiting the evolution of nonradiative supernova remnants: A hydrodynamical-informed parameterization of the shock positions
R. Bandiera, N. Bucciantini, J. Martín +2
Understanding the evolution of a supernova remnant shell in time is fundamental. Such understanding is critical to build reliable models of the dynamics of the supernova remnant sh…