2,368 research outputs found
High Energy Phenomena in Blazars
Advances in the capabilities of X-ray, gamma-ray and TeV telescopes have
brought new information on the physics of relativistic jets, which are
responsible for the blazar "phenomenon". In particular the broad band
sensitivity of the BeppoSAX satellite, extending up to 100 KeV has allowed
unprecedented studies of their hard X-ray spectra. I summarize here some basic
results and present a unified view of the blazar population, whereby all
sources contain essentially similar jets despite diversities in other
properties, like the presence or absence of emission lines in their optical
spectra. Blazars with emission lines are of particular interest in that it is
possible to estimate both the luminosity of the jet and the luminosity of the
accretion disk. Implications for the origin of the power carried by
relativistic jets, possibly involving rapidly spinning supermassive black holes
are discussed. We suggest that emission line blazars are accreting at near
critical rates, while BL lacs, where emission lines are weak or absent are
highly subcritical.Comment: 11 pages, 7 figures, presented at the 20th Texas Symposium, 10-15
Dec. 200
High Energy Phenomena in Clusters of Galaxies
Several phenomena in high energy astrophysics have been recently related to
clusters of galaxies and to cosmic ray interactions occurring inside these
structures. In many of these phenomena the observable effects depend on the
energy density of cosmic rays confined in the Intra Cluster (IC) medium, which
is a poorly known quantity. We propose here that useful indications about this
quantity can be obtained from present and future observations of galaxy
clusters in the radio and hard X-ray frequency ranges.Comment: 5 pages, 3 Figures, Latex (using espcrc2,epsfig), to appear in the
Proceedings of the TAUP97, Eds. A. DiCredico et al., in press. Send comments
to S.Colafrancesco: [email protected]
High Energy Phenomena in Supergiant X-ray Binaries
The INTEGRAL satellite has revealed a major population of supergiant High
Mass X-ray Binaries in our Galaxy, revolutionizing our understanding of binary
systems and their evolution. This population, constituted of a compact object
orbiting around a massive and luminous supergiant star, exhibits unusual
properties, either being extremely absorbed, or showing very short and intense
flares. An intensive set of multi-wavelength observations has led us to reveal
their nature, and to show that these systems are wind-fed accretors, closely
related to massive star-forming regions. In this paper I describe the
characteristics of these sources, showing that this newly revealed population
is linked to the evolution of gamma-ray emitting massive stars with a compact
companion.Comment: Contributed talk to "High Energy Phenomena in Massive Stars"
Workshop, held in Jaen, Spain, Feb. 2009. To be published in ASP conf.
series; Editors: Marti, Josep, 9 pages, 2 figure
High Energy Phenomena on the Sun
The proceedings of a symposium of high energy phenomena on the sun are presented. The subjects discussed include the following: (1) flare theories and optical observations, (2) microwave and hard X-ray observations, (3) ultraviolet and soft X-ray emissions, (4) nuclear reactions in solar flares, (5) energetic particles from the sun, (6) magnetic fields and particle storage, and (7) radio emissions in the corona and interplanetary space
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