40 citations · 40 across the 2 of their papers we have counts for
2 papers
astro-ph.HE2024
Time evolution of the synchrotron X-ray emission in Kepler's SNR: the effects of turbulence and shock velocity
Vincenzo Sapienza, Marco Miceli, Oleh Petruk +5
The maximum energy of electrons in supernova remnant (SNR) shocks is typically limited by radiative losses, where the synchrotron cooling time equals the acceleration time. The low…
astro-ph2005★ 40 cited
Time Variability in the X-ray Nebula Powered by Pulsar B1509-58
T. DeLaney, B. M. Gaensler, J. Arons +1
We use new and archival Chandra and ROSAT data to study the time variability of the X-ray emission from the pulsar wind nebula (PWN) powered by PSR B1509-58 on timescales of one we…