Berezinsky and Prilutsky analyzed one possible mechanism for their formation, based on (*) neutrino-antineutrino annihilation, while Prilutsky and Usov developed the first cosmological model of them, using active galactic nuclei.
A catalog of these objects was published by Mazets, who analyzed data from the KONUS experiment, while another was published by Fishman using data from the BATSE experiment. Lamb and Paczynski participated in a 1995 debate about their location. Berezinsky and Prilutsky analyzed one possible mechanism for their formation, based on (*) neutrino-antineutrino annihilation, while Prilutsky and Usov developed the first cosmological model of them, using active galactic nuclei. The BeppoSAX experiment discovered the first x-ray afterglow in these objects, discovered by Klebesadel et al while analyzing data from the Vela satellites, whose original purpose was to watch for nuclear tests. For 10 points, name these intense flashes of the namesake uncharged radiation.
A catalog of these objects was published by Mazets, who analyzed data from the KONUS experiment, while another was published by Fishman using data from the BATSE experiment.
{gamma ray burst}s [accept {gamma ray burster}s; accept {GRB}s] (3)