HAL (France)
open access
Studying gamma-ray halos around pulsars using H.E.S.S. data
Pulsars produce emission nebulae wherein electrons and positrons are confined in a nebular magnetic field originating in the pulsar. Such pulsar wind nebulae constitute a prominent category of gamma-ray sources and are possibly important contributors to the local positron cosmic-ray spectrum. Escape
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Assessing the detectability and identification of pulsar halos with H.E.S.S. and CTAO#1131071
- Spectral energy-loss bump and $γ$-ray pulsar halos#635836
- Spectral energy-loss bump and $γ$-ray pulsar halos#633487
- The problem of the puer aeternus#1289849
- A Cadet of the Black Star Line#58887
Record · ID 1367050
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive