61 citations · 797 across the 51 of their papers we have counts for
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Deciphering the Nature of the Pulsar Wind Nebula CTB 87 with XMM-Newton
Benson Guest, Samar Safi-Harb, Austin MacMaster +5
CTB 87 (G74.9+1.2) is an evolved supernova remnant (SNR) which hosts a peculiar pulsar wind nebula (PWN). The X-ray peak is offset from that observed in radio and lies towards the…
On the origin of jet-like features in bow shock pulsar wind nebulae
Barbara Olmi, Niccolò Bucciantini
Bow shock pulsar wind nebulae are a large class of non-thermal synchrotron sources associated to old pulsars, that have emerged from their parent supernova remnant and are directly…
Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: emission and polarization
B. Olmi, N. Bucciantini
Bow shock pulsar wind nebulae are observed with a variety of complex morphologies at different wavelengths, most likely due to differences in the magnetic field strength and pulsar…
Full-3D relativistic MHD simulations of Bow Shock Pulsar Wind Nebulae: dynamics
Barbara Olmi, Niccolo' Bucciantini
Bow shock pulsar wind nebulae (BSPWNe) are know to show a large variety of shapes and morphologies, both when comparing different objects, and for the same object in different ener…