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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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Gamma Ray Sources and Techniques for Gamma Ray Radiology [PDF]
J. J. Hirschfield+2 more
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American Cancer Society nutrition and physical activity guideline for cancer survivors
Ca-A Cancer Journal for Clinicians, 2022Cheryl L Rock+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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Spacecraft Navigation Using Celestial Gamma-Ray Sources
, 2015Chuck S. Hisamoto, S. Sheikh
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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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“Gamma — Ray Sources in our Galaxy”
1987Astronomy with gamma-rays in the tens of MeV-few GeV energy region was started in the sixties, with the availability of reasonable space vehicles, in the hope of opening a new window of observational astronomy which was to shed new “light” on a variety of energetic astrophisical processes in compact objects as well as in the interstellar medium (ISM).
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