A Systematic Search for MeV–GeV Pulsar Wind Nebulae without Gamma-Ray Detected Pulsars
An increasing number of pulsar wind nebulae (PWNe) are being identified in the TeV band by ground-based Imaging Air Cherenkov Telescopes such that they constitute the dominant source class of Galactic TeV emitters. However, MeV–GeV PWN counterparts are still largely lacking. To date, only a dozen PW...
Saved in:
Similar Items
-
Discovery and Timing of Four γ-Ray Millisecond Pulsars
by: M. Kerr, et al.
Published: (2025-01-01) -
Puzzling Variation of Gamma Rays from the Sun over the Solar Cycle Revealed with Fermi-LAT
by: A. Acharyya, et al.
Published: (2025-01-01) -
Investigating the Spectral Nature of Gigahertz-peaked Spectra Pulsar Candidates
by: K. Rożko, et al.
Published: (2025-01-01) -
Aspergillosis in domestic and wild birds in northeastern Brazil: 2000-2022
by: E.P.F. Souto, et al.
Published: (2025-04-01) -
The Mass of the Vela Pulsar Progenitor and the Age of the Vela-Puppis Complex
by: Jeremiah W. Murphy, et al.
Published: (2025-01-01)