Not exact matches
Quick follow - up observations undertaken with the 8.2 -
m Antu instrument
at European Southern Observatory's Very
Large Telescope in the Paranal and the 1.5 - meter Danish telescope
at La Silla identified a faint, point - like object in visible light that
was fading rapidly, the optical counterpart of the
gamma - ray burst called the «afterglow» (Pedersen et al, 2000).
His experience on X-ray and
Gamma ray detectors has
been gained in particular as technical coordinator of the two
largest ever built calorimeters for the L3 experiment in the eighties
at the
large electron - positron ring (LEP)
at CERN under the leadership of the Nobel laureate Prof. Samuel Ting, with 12» 000 Bismuth Germanate (BGO) crystals (1.5 tons), and for the CMS experiment
at the
large hadron collider (LHC)
at CERN starting in 2008, with 76» 000 Lead Tungstate (PWO) crystals (100 tons).
Since
gamma radiation provides the energy preventing gravitational collapse of the outer layers of the star onto the core,
at some point the loss of this energy (through so - called «pair instability») causes violent pulsations that eject a
large fraction of the outer layers of the star and eventually a star's outer layers to collapse inward to create a thermonuclear explosion that, in theory, would
be brighter than previously detected supernova.
This
is quite a
large move in the Delta and thus shows how
at the money options have the most
Gamma.