TL;DR
This paper discusses gamma-ray binaries, a class of high-energy sources in the Milky Way, highlighting the challenges in identifying them due to telescope resolution limitations and the new insights gained from recent observations.
Contribution
The paper provides a comprehensive overview of gamma-ray binaries, emphasizing recent observational advances and the importance of improved resolution in identifying these sources.
Findings
Identification of gamma-ray binaries as a distinct class
Recent telescopic observations have expanded known sources
Challenges remain in resolving and classifying gamma-ray sources
Abstract
Recent ground based and space telescopes that detect high energy photons from a few up to hundreds of gigaelectron volts (GeV) have opened a new window on the universe. However, because of the relatively poor angular resolution of these telescopes, a large fraction of the thousands of sources of gamma-rays observed remains unknown. Compact astrophysical objects are among those high energy sources, and in the Milky Way there is a particular class called "Gamma-Ray Binaries".
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.