A population synthesis study with a hybrid TIDE+L dynamical model predicts that the Cherenkov Telescope Array Observatory will detect roughly ten times more Galactic pulsar wind nebulae than are currently known in TeV gamma rays.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2verdicts
UNVERDICTED 2representative citing papers
Population synthesis of normal radio pulsars finds that exponential magnetic field decay with timescale 8.3 Myr reproduces observed distributions of P, P-dot, DM and flux better than power-law decay.
citing papers explorer
-
Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
A population synthesis study with a hybrid TIDE+L dynamical model predicts that the Cherenkov Telescope Array Observatory will detect roughly ten times more Galactic pulsar wind nebulae than are currently known in TeV gamma rays.
-
Pulsar Population Synthesis with Magnetorotational Evolution: Constraining the Decay of Magnetic field
Population synthesis of normal radio pulsars finds that exponential magnetic field decay with timescale 8.3 Myr reproduces observed distributions of P, P-dot, DM and flux better than power-law decay.