Orbital Modulation of Gamma Rays up to 100 TeV from LS 5039
Gamma-ray binaries are luminous in gamma rays, composed of a compact object orbiting a massive companion star. The interaction between these two objects can drive relativistic outflows, either jets or winds, in which particles can be accelerated to energies reaching hundreds of teraelectronvolts (Te...
| Published in: | The Astrophysical Journal Letters |
|---|---|
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/ade760 |
