Global ETD Search
Search theses and dissertations gathered from participating repositories worldwide. Every result links back to the library that holds it. No account is needed.
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Showing 1 to 6 of 6 for “"gamma-ray emitters"”.
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Calculation of absorbed fraction for internal gamma-ray emitters.
Massachusetts Institute of Technology. Dept. of Nuclear Engineering. Thesis. 1974. M.S.
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Supernovae as gamma ray emitters from the MeV to the TeV
"Gamma rays offer unique probes of supernovae as cosmic-ray accelerators and as nucleosynthesis sites. My thesis work focuses on how to explore these two aspects of supernovae. (1) Both starburst galaxies and ultra luminous infrared galaxies are new gamma-ray source classes discovered by Fermi and …
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Gamma-Ray Observations of X-ray Binaries
<p>The detection of GeV/TeV emission from X-ray binaries (XRBs) has established a new class of high-energy (HE, >0.1 GeV) and very-high-energy (VHE, >100 GeV) gamma-ray emitters. XRBs are formed by a compact object, either a neutron star or a black hole, and by an optical companion star. Some XRBs …
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Investigating Extended Gamma-Ray Sources with ASTRI and CTAO: Observation, Analysis and Modelling
This thesis investigates the gamma-ray emission from Galactic sources with next-generation IACTs (Imaging Atmospheric Cherenkov Telescopes) like the telescopes of the ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array and CTAO (Cherenkov Telescope Array Observatory), with …
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Investigating Extended Gamma-Ray Sources with ASTRI and CTAO: Observation, Analysis and Modelling
This thesis investigates the gamma-ray emission from Galactic sources with next-generation IACTs (Imaging Atmospheric Cherenkov Telescopes) like the telescopes of the ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array and CTAO (Cherenkov Telescope Array Observatory), with …
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Pulsar wind nebulae at high energies
… wind nebulae (PWNe) are the most abundant TeV gamma-ray emitters in the Milky Way. The radiative emission of these objects is powered by fast-rotating pulsars, which donate parts of their rotational energy into winds of relativistic particles. This thesis presents an in-depth study of the …