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Acceleration of particles in Gamma Ray sources: Blazars and Gamma Ray Bursts
AIP Conference Proceedings, 2001The objectives of my talk are to indicate the requirements for particle acceleration for both electrodynamic models and hadronic models in blazars, then to propose a relativistic Fermi acceleration process to achieve the goal of UHE Cosmic Ray production in relativistic flows.
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VHE and UHE Gamma Ray Sources [PDF]
The observations of Very High Energy, VHE, and Ultra High Energy, UHE, gamma rays from celestial sources are reviewed. Cerenkov detectors for VHE gamma ray measurements and extended air shower arrays for UHE measurements are described. The x-ray binary pulsar source VHE and UHE observations of Cyg X-3, Her X-1, Vela X-1 and Cen X-3 and of the radio ...
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Gamma Ray Sources and Techniques for Gamma Ray Radiology [PDF]
J. J. Hirschfield+2 more
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An overview of real‐world data sources for oncology and considerations for research
Ca-A Cancer Journal for Clinicians, 2022Lynne T Penberthy+2 more
exaly
American Cancer Society nutrition and physical activity guideline for cancer survivors
Ca-A Cancer Journal for Clinicians, 2022Tracy E Crane+2 more
exaly
1992
The ubiquitous nature of cosmic X-ray sources was not fully realized until satellites such as Uhuru, Ariel, HEAO and Einstein surveyed the X-ray sky. For instance, the fourth Uhuru (the Swahili word for freedom) catalogue contains 339 X-ray sources in the photon energy range 2 to 6 keV (1 keV = 103 eV = 1.6 × 109erg), while one HEAO (High Energy ...
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The ubiquitous nature of cosmic X-ray sources was not fully realized until satellites such as Uhuru, Ariel, HEAO and Einstein surveyed the X-ray sky. For instance, the fourth Uhuru (the Swahili word for freedom) catalogue contains 339 X-ray sources in the photon energy range 2 to 6 keV (1 keV = 103 eV = 1.6 × 109erg), while one HEAO (High Energy ...
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Unidentified Gamma-Ray Sources: An Introduction
2001What makes a gamma-ray source “unidentified”? Typical gamma-ray source error boxes are large by astronomical standards; therefore a positional correlation with a known object is usually not enough to identify a source. Historically, identifications have come in several ways: (1) finding a time-variable signal seen at another wavelength; (2) repeatedly ...
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