Gamma-ray Bursts, Their High Energy Emission as Observed by EGRET
Author | : María Magdalena González Sánchez |
Publisher | : |
Total Pages | : 206 |
Release | : 2005 |
Genre | : |
ISBN | : |
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Author | : María Magdalena González Sánchez |
Publisher | : |
Total Pages | : 206 |
Release | : 2005 |
Genre | : |
ISBN | : |
Author | : Marco Maria Massai |
Publisher | : World Scientific |
Total Pages | : 251 |
Release | : 2007-10-02 |
Genre | : Science |
ISBN | : 9814474495 |
The research program in gamma-ray astronomy focuses on increasing our knowledge of the nature and origin of galactic and extragalactic gamma rays, and understanding high-energy processes in the Sun, celestial objects, interstellar medium, and extragalactic space.This book not only provides an overview of the latest research and future plans for space-borne and ground-based experiments dedicated to the observation of the gamma-ray sky, but also addresses the topic of variable gamma-ray sources from the perspective of their identification and counterparts at different wavelengths. It further gives an overview of the theory related to the most qualified emission processes that take place in these sources and of the nature of their variability.
Author | : Cheng Ho |
Publisher | : Cambridge University Press |
Total Pages | : 532 |
Release | : 1992-03-12 |
Genre | : Nature |
ISBN | : 9780521414494 |
Summarizes the current understanding of Astronomical gamma-ray bursts, short-lived flashes of high-energy radiation, which have eluded even a basic explanation for over twenty years, and describes directions for future research.
Author | : Bing Zhang |
Publisher | : Cambridge University Press |
Total Pages | : 617 |
Release | : 2019 |
Genre | : History |
ISBN | : 1107027616 |
A complete text on the physics of gamma-ray bursts, the most brilliant explosions since the Big Bang.
Author | : Gilbert Vedrenne |
Publisher | : Springer Science & Business Media |
Total Pages | : 613 |
Release | : 2009-03-20 |
Genre | : Science |
ISBN | : 354039088X |
Since their discovery was first announced in 1973, gamma-ray bursts (GRBs) have been among the most fascination objects in the universe. While the initial mystery has gone, the fascination continues, sustained by the close connection linking GRBs with some of the most fundamental topics in modern astrophysics and cosmology. Both authors have been active in GRB observations for over two decades and have produced an outstanding account on both the history and the perspectives of GRB research.
Author | : Chryssa Kouveliotou |
Publisher | : Cambridge University Press |
Total Pages | : 361 |
Release | : 2012-11-22 |
Genre | : Science |
ISBN | : 1139576488 |
Cosmic gamma ray bursts (GRBs) have fascinated scientists and the public alike since their discovery in the late 1960s. Their story is told here by some of the scientists who participated in their discovery and, after many decades of false starts, solved the problem of their origin. Fourteen chapters by active researchers in the field present a detailed history of the discovery, a comprehensive theoretical description of GRB central engine and emission models, a discussion of GRB host galaxies and a guide to how GRBs can be used as cosmological tools. Observations are grouped into three sets from the satellites CGRO, BeppoSAX and Swift, and followed by a discussion of multi-wavelength observations. This is the first edited volume on GRB astrophysics that presents a fully comprehensive review of the subject. Utilizing the latest research, Gamma-ray Bursts is an essential desktop companion for graduate students and researchers in astrophysics.
Author | : |
Publisher | : |
Total Pages | : |
Release | : 2011 |
Genre | : |
ISBN | : |
Gamma-ray bursts (GRBs) are short and intense emission of soft [gamma]-rays, which have fascinated astronomers and astrophysicists since their unexpected discovery in 1960s. The X-ray/optical/radio afterglow observations confirm the cosmological origin of GRBs, support the fireball model, and imply a long-activity of the central engine. The high-energy [gamma]-ray emission (> 20 MeV) from GRBs is particularly important because they shed some lights on the radiation mechanisms and can help us to constrain the physical processes giving rise to the early afterglows. In this work, we review observational and theoretical studies of the high-energy emission from GRBs. Special attention is given to the expected high-energy emission signatures accompanying the canonical early-time X-ray afterglow that was observed by the Swift X-ray Telescope. We also discuss the detection prospect of the upcoming GLAST satellite and the current ground-based Cerenkov detectors.