Results 201 to 210 of about 1,645,326 (221)
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Physics Bulletin, 1970
T C Weeks London: Chapman and Hall 1969 pp xi + 209 price £3 This is the first comprehensive book on a new and exciting subject - high energy astrophysics. The name of this subject has a double meaning: it refers to the existence of celestial processes in which very large amounts of total energy are explosively released (up to 1060 erg or more), and to
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T C Weeks London: Chapman and Hall 1969 pp xi + 209 price £3 This is the first comprehensive book on a new and exciting subject - high energy astrophysics. The name of this subject has a double meaning: it refers to the existence of celestial processes in which very large amounts of total energy are explosively released (up to 1060 erg or more), and to
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High energy astrophysics missions
Space 2000 Conference and Exposition, 2000NASA’s Structure and Evolution of the Universe (SEU) program uses X-ray and Gamma ray observations to observe the extremes of gravity throughout the universe. This program will probe the nature of black holes, ultimately obtaining a direct image of the event horizon.
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1985
In view of the broad range of topics covered by Commission 48 and the consequent inevitable overlap with other commissions, it is not feasible to produce a comprehensive self-contained report. The commission therefore restricts its report to a selected list of accessible recent review articles and conference reports, where up-to-date summaries of ...
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In view of the broad range of topics covered by Commission 48 and the consequent inevitable overlap with other commissions, it is not feasible to produce a comprehensive self-contained report. The commission therefore restricts its report to a selected list of accessible recent review articles and conference reports, where up-to-date summaries of ...
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1973
This report concentrates on three observational areas where progress during the last 3 years has been especially noteworthy. These are: X-ray astronomy (reviewed by H. Gursky), γ-ray astronomy (reviewed by G. Fazio) and Cosmic rays (reviewed by M. Shapiro and R. Silberberg). Gratitude is expressed to these contributors, and to Dr J. D.
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This report concentrates on three observational areas where progress during the last 3 years has been especially noteworthy. These are: X-ray astronomy (reviewed by H. Gursky), γ-ray astronomy (reviewed by G. Fazio) and Cosmic rays (reviewed by M. Shapiro and R. Silberberg). Gratitude is expressed to these contributors, and to Dr J. D.
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1980
Jan Oort is the same age as our century, the century or brilliant astronomic discoveries. Contemporaries, true, are apt to underestimate the achievements of the past and to attach particular importance to the events they witness. In fact, however, astronomy and physics began rapidly developing more than three hundred years ago and there is no ground to
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Jan Oort is the same age as our century, the century or brilliant astronomic discoveries. Contemporaries, true, are apt to underestimate the achievements of the past and to attach particular importance to the events they witness. In fact, however, astronomy and physics began rapidly developing more than three hundred years ago and there is no ground to
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Astrophysical High Energy Neutrinos
AIP Conference Proceedings, 2007Astrophysical candidate sources of ultrahigh‐energy cosmic‐rays are also expected to produce high‐energy neutrinos in situ and around their acceleration sites by interacting with abundant soft photons or nucleons. Detection of these neutrinos then may identify the yet unknown sources of the cosmic rays.
Soebur Razzaque, Jeffrey R. Wilkes
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Aspects Of High Energy Astrophysics
Publications of the Astronomical Society of Australia, 1972Observational astronomy extends, in terms of energy in the electromagnetic spectrum, from below 10-8eV to above 108eV. Studies of cosmic rays extend this range to the neighbourhood of 1019eV (about a Joule) and the aspects of high energy astrophysics discussed in the present paper are those concerned with cosmic rays of energy upwards of about 1015eV.
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High-Energy Neutrino Astrophysics
2014Neutrino astronomy shares with \(\upgamma \)-ray astronomy the objective of understanding the sources and mechanisms of CR acceleration. Due to their much larger interaction cross section, \(\upgamma \)-rays are easier to detect than neutrinos, and \(\upgamma \)-ray astronomy is having a fundamental importance on several topical areas of modern ...
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Currents in High-Energy Astrophysics
1995I Cosmic Gamma Rays, X-Rays, and Neutrinos: The Sky as Viewed from the Compton Gamma-Ray Observatory, G. Kanbach Cosmic Gamma-Ray Bursts, M. Baring Gamma-Ray Production in the Winds of Wolf-Rayet Stars, P.J. Meintjes, G. Kanbach Origin of High-Energy X-Ray Emission from NGC 253, O. Goldshmidt Spectral and Temporal Variability in Low-Mass X-Ray Binaries,
Maurice M. Shapiro +2 more
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Very high energy astrophysics with the SHALON Cherenkov telescopes
, 2020V. G. Sinitsyna +5 more
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