Gamma-ray bursts 2007: proceedings of the Santa Fe conference : Santa Fe, New Mexico, 5-9 November 2007
For more than three decades, gamma-ray bursts have grown from an oddity to a central topic in astrophysics. Not only are they the largest explosions since the big bang, capable of flooding most of the universe with gamma-rays, but their brilliance serves as a backlight that can illuminate the cosmos far deeper into the early universe than any other object. Their unpredictability has forced researchers to use extreme measures to observe them: completely autonomous satellites and robotic ground-based telescopes. Their bizarre physical properties have required new theories on massive explosions.
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Status of Swift GRB Observations
GammaRay Bursts Classified Physically
On the Selection Effects of the pek10Correlation
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2008 American Institute analysis arXiv Astronomy Astrophys Astrophysics BATSE BeppoSAX Bursa central engine collapsar component correlation decay density detected detectors distribution duration edited electrons energy band Fenimore O 2008 FIGURE fireball flares fluence flux function Fynbo Galactic Galassi gamma gamma-ray bursts gamma-ray bursts GRBs Gehrels GLAST GRB afterglows GRB Coordinates Network GRB host high energy host galaxy hypernovae images Institute of Physics internal shock isotropic jet break Keywords light curve long GRBs Lorentz factor luminosity magnetic field magnitude Meszaros neutrino neutron star Observatory observed optical afterglow outflow PACS Palmer panel parameters peak energy phase photon power-law progenitor prompt emission pulse radiation redshift relativistic relativistic jets RHESSI sample Santa Ft shell short GRBs shows simulations spectral evolution spectrum star supernova Swift GRBs synchrotron telescope temporal trigger University UVOT variability X-ray afterglow y-ray Zhang