Pulsar wind nebulae with bow shocks: non-thermal radiation and cosmic ray leptons
AM Bykov, E Amato, AE Petrov… - Space Science …, 2017 - Springer
Pulsars with high spin-down power produce relativistic winds radiating a non-negligible
fraction of this power over the whole electromagnetic range from radio to gamma-rays in the …
fraction of this power over the whole electromagnetic range from radio to gamma-rays in the …
Gamma-ray pulsar revolution
PA Caraveo - Annual Review of Astronomy and Astrophysics, 2014 - annualreviews.org
Isolated neutron stars (INSs) were the first sources identified in the field of high-energy
gamma-ray astronomy. In the 1970s, only two sources had been identified, the Crab and …
gamma-ray astronomy. In the 1970s, only two sources had been identified, the Crab and …
The second Fermi Large Area Telescope catalog of gamma-ray pulsars
This catalog summarizes 117 high-confidence⩾ 0. 1 GeV gamma-ray pulsar detections
using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite …
using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite …
Pulsar-wind nebulae: Recent progress in observations and theory
O Kargaltsev, B Cerutti, Y Lyubarsky, E Striani - Space Science Reviews, 2015 - Springer
In this review we describe recent observational and theoretical developments in our
understanding of pulsar winds and pulsar-wind nebulae (PWNe). We put special emphasis …
understanding of pulsar winds and pulsar-wind nebulae (PWNe). We put special emphasis …
Fermi-LAT search for pulsar wind nebulae around gamma-ray pulsars
The high sensitivity of the Fermi-LAT (Large Area Telescope) offers the first opportunity to
study faint and extended GeV sources such as pulsar wind nebulae (PWNe). After one year …
study faint and extended GeV sources such as pulsar wind nebulae (PWNe). After one year …
Probing the extent of the non-thermal emission from the Vela X region at TeV energies with HESS
A Abramowski, F Acero, F Aharonian… - Astronomy & …, 2012 - aanda.org
Context. Vela X is a region of extended radio emission in the western part of the Vela
constellation: one of the nearest pulsar wind nebulae, and associated with the energetic …
constellation: one of the nearest pulsar wind nebulae, and associated with the energetic …
Fermi Large Area Telescope observations of the Vela-X pulsar wind nebula
We report on gamma-ray observations in the off-pulse window of the Vela pulsar PSR
B0833− 45 using 11 months of survey data from the Fermi Large Area Telescope (LAT). This …
B0833− 45 using 11 months of survey data from the Fermi Large Area Telescope (LAT). This …
FERMI DETECTION OF THE PULSAR WIND NEBULA HESS J1640− 465
We present observations of HESS J1640− 465 with the Fermi-Large Area Telescope. The
source is detected with high confidence as an emitter of high-energy gamma-rays. The …
source is detected with high confidence as an emitter of high-energy gamma-rays. The …
The Vela-X pulsar wind nebula revisited with four years of Fermi Large Area Telescope observations
MH Grondin, RW Romani… - The Astrophysical …, 2013 - iopscience.iop.org
The Vela supernova remnant (SNR) is the closest SNR to Earth containing an active pulsar,
the Vela pulsar (PSR B0833− 45). This pulsar is an archetype of the middle-aged pulsar …
the Vela pulsar (PSR B0833− 45). This pulsar is an archetype of the middle-aged pulsar …
First Emulsion γ-Ray Telescope Imaging of the Vela Pulsar by the GRAINE 2018 Balloon-borne Experiment
S Takahashi, S Aoki, A Iyono, A Karasuno… - The Astrophysical …, 2023 - iopscience.iop.org
We are developing the Gamma-Ray Astro-Imager with Nuclear Emulsion project, designed
for 10 MeV–100 GeV cosmic γ-ray observations with a high angular resolution (5'/0 fdg 08 at …
for 10 MeV–100 GeV cosmic γ-ray observations with a high angular resolution (5'/0 fdg 08 at …