Results 181 to 190 of about 16,751 (259)
invited talk at the Workshop "Blazar Demographics and Physics" Baltimore, July 2000, ASP Conf. Series, P. Padovani and C. M. Urry eds., in press. (6 pages, LaTex, 10 PostScript figures, uses newpasp.sty).
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Extreme Electron Acceleration with Fixed Radiation Energy. [PDF]
Good MRR, Singha C, Zarikas V.
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This review paper discusses the past and present observations of gamma-ray blazars with both space and ground-based gamma-ray telescopes (such as EGRET and current TeV telescopes), and with the VLBA. I also discuss the more sensitive gamma-ray telescopes such as AGILE and GLAST that will become available over the next several years, and how ...
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A wind environment and Lorentz factors of tens explain gamma-ray bursts X-ray plateau. [PDF]
Dereli-Bégué H +5 more
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Characterizing the Solar Activity Using the Visibility Graph Method. [PDF]
Zurita-Valencia T, Muñoz V.
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Gamma-ray flares from relativistic magnetic reconnection in the jet of the quasar 3C 279. [PDF]
Shukla A, Mannheim K.
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A ring-like accretion structure in M87 connecting its black hole and jet. [PDF]
Lu RS +120 more
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Considering light-matter interactions in the Friedmann equations. [PDF]
Vavryčuk V.
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Considering shock-accelerated protons in addition to electrons in a synchrotron radio jet naturally produces the observed X- through gamma ray continuum emission of flat-spectrum radio-loud AGN, whereas the corresponding shock-accelerated electrons produce the infrared through optical continuum.
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Core Concept: Multimessenger astronomy probes deep-space events with an arsenal of lenses. [PDF]
Ornes S.
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