Galactic Compact Objects Section of the White Paper on the Status and Future of Ground-based TeV Gamma-ray Astronomy
P. Kaaret, A. A. Abdo, J. Arons, M. Baring, W. Cui, B. Dingus, J., Finley, S. Funk, S. Heinz, B. Gaensler, A. Harding, E. Hays, J. Holder, D., Kieda, A. Konopelko, S. LeBohec, A. Levinson, I. Moskalenko, R. Mukherjee, R., Ong, M. Pohl, K. Ragan, P. Slane, A. Smith, D. Torres

TL;DR
This white paper section reviews how upcoming ground-based TeV gamma-ray experiments can enhance understanding of Galactic compact objects like pulsars and X-ray binaries, highlighting future research directions.
Contribution
It provides a comprehensive overview of the potential scientific advancements in Galactic compact objects through future gamma-ray observations.
Findings
Future experiments will improve detection sensitivity.
Enhanced observations will clarify emission mechanisms.
New data will refine models of compact objects.
Abstract
This is a report on the findings of the Galactic compact objects working group for the white paper on the status and future of TeV gamma-ray astronomy. The white paper is an APS commissioned document, and the full version has also been released and can be found on astro-ph. This section of the white paper discusses the potential of future ground-based gamma-ray experiments to advance our understanding of the physics of Galactic compact objects including pulsars, pulsar wind nebulae, and X-ray binaries.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Particle Detector Development and Performance
