Astronomy & Space Science · AST-863
Chandra, Fermi & High-Energy Observatories: Physical Mechanisms
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Mechanism
Mechanism of Chandra, Fermi & High-Energy Observatories
X-rays often arise from thermal plasma or high-energy electron processes, while gamma rays can be produced by particle interactions, nuclear transitions, inverse Compton scattering, or extreme transients. Detector designs convert incoming high-energy photons into measurable particle cascades or charge signals.
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References & evidence
Source library for this chapter
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- 01Chandra X-ray ObservatoryOpen source ↗
NASA Science
- 02Fermi Gamma-ray Space TelescopeOpen source ↗
NASA Science
View claim-by-claim traceability3 verified claims
High-energy observatories detect X-rays and gamma rays produced in hot plasma, shocks, neutron stars, black-hole accretion flows, radioactive processes, and relativistic particle populations.
supported · checked Sep 22, 2026Chandra resolves supernova remnants, clusters, jets, and compact binaries; Fermi maps pulsars, active galaxies, gamma-ray bursts, diffuse emission, and high-energy transients.
supported · checked Sep 22, 2026X-rays often arise from thermal plasma or high-energy electron processes, while gamma rays can be produced by particle interactions, nuclear transitions, inverse Compton scattering, or extreme transients.
supported · checked Sep 22, 2026