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Basic informations about GRBs


Gamma-Ray Bursts (GRBs) are very short and intense pulses of soft gamma-rays. Typical burst lasts from a fraction of a second to several hundred seconds. GRBs arrive from random directions in the sky. In gamma-rays, GRBs are the most luminous sources on the sky. Total energy, emitted during the burst (assuming spherical explosion) is of the order of ~10^49 - 10^51 erg. To emit such an amount of energy the Sun should shine from one billion to 100 billions years!

GRBs were discovered in 1967 by instruments of Vela mission satelite. This spacecraft was launched by the U.S. Department of Defense to search for nuclear explosions violating the Nuclear Test Ban Treaty. Soon after launching, the instrument detected the first event of gamma-ray burst, but this result was published 6 years later in 1973. Detailed study of these bursts revealed that they did not come neither from the Earth nor from the close Solar System and that they were a totally new class of cosmic objects. Today we know a lot about GRBs but they still keep many mysteries.



Last modification: , 2010-09-05
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Charles University, PragueAstronomical Observatory, Ondrejov, CZECHCSNSMMPEUniversität WürzburgKonkoly ObservatoryBudapest UniversityUCDCNRIPJSkobeltsyn Institut, Moscow, RUSSIAIKI