Flux Evolution of PSR B0540--69 and the Spectral Energy Distribution of its Pulsar Wind Nebula
astro-ph.HE
Submitted: 2026-10-09
Updated: 2026-10-09
Comments: 11 pages, 5 figures, 5 tables, submitted
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Sources
- Radio and X-ray Observations of PSR B0540-69
- The optical light curve of the LMC pulsar B0540-69 in 2009
- The first ultraviolet detection of the Large Magellanic Cloud pulsar PSR B0540-69 and its multi-wavelength properties
- X-ray Phase-Resolved Spectroscopy of PSRs B0531+21, B1509-58, and B0540-69 with RXTE
- A distance to the Large Magellanic Cloud that is precise to one per cent
- A spatially resolved plerionic X-ray nebula around PSR B0540-69
- Discovery of a Spin-Down State Change in the LMC Pulsar B0540-69
- New Phase-coherent Measurements of Pulsar Braking Indices
- Long-term timing and emission behavior of the young Crab-like pulsar PSR B0540-69
- The brightening of the pulsar wind nebula of PSR B0540--69 after its spin-down rate transition
- The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition
- A growing braking index and spin-down swings for the pulsar PSR B0540-69
- New and updated timing models for seven young energetic X-ray pulsars, including the Big Glitcher PSR J0537-6910
- Spin-down changes in PSR B0540-69 induced by a drift of the magnetic axis
- On the new braking index of PSR B0540-69: further support for magnetic field growth of neutron stars following submergence by fallback accretion
- Gamma-ray flares from pulsar wind nebulae in the Large Magellanic Cloud
- Discovery of Powerful Gamma-Ray Flares from the Crab Nebula
- Gamma-ray flares from the Crab Nebula
- Gamma-ray Activity in the Crab Nebula: The Exceptional Flare of April 2011
- Peta-electron volt gamma-ray emission from the Crab Nebula
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