arXiv (All)
open access
Gamma-ray Emission from the S147 Region: Indication of Escaping Cosmic Rays Interacting with Molecular Clouds
We present a detailed analysis of $γ$-ray emission from the middle-aged supernova remnant (SNR) S147 (G180.0$-$1.7) using approximately 16.5 years of Fermi-LAT data. Spatially, a new extended $γ$-ray component distinct from the emission associated with the H$α$ filaments of the SNR shell is identifi
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
- Investigating Fermi-LAT data to find gev gamma-ray counterparts of new candidate radio supernova remnants detected in the GLEAM survey#455593
- A Significant Dust Reservoir Uncovered with JWST in the Type Ic SN 1983V More Than 40 Years Post-Explosion#1013861
- Reconstructing Gamma Ray Burst Energy Relations with Observational H(z) data in Neural Network Framework#1084111
- Supernova 1987A was a "failed supernova" twenty thousand years before its jet-driven explosion#684618
- Supernova 1987A was a "failed supernova" twenty thousand years before its jet-driven explosion#682840
Record · ID 987576
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