A population synthesis study with a hybrid TIDE+L dynamical model predicts that the Cherenkov Telescope Array Observatory will detect roughly ten times more Galactic pulsar wind nebulae than are currently known in TeV gamma rays.
Review on the Observed and Physical Properties of Core Collapse Supernovae
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abstract
This paper summarizes observed and physical properties of all types of core collapse supernovae. Despite the great diversity displayed by these objects, several regularities emerge which suggest that 1) there is a continuum in the properties of these objects, 2) the mass of the envelope is one of the driving parameters of the explosion, or it is correlated with some other property of the core, with the latter determining the outcome of the explosion, and 3) the physics of the core and explosion mechanism of all core collapse supernovae are not be fundamentally different, regardless of the external appearance of the supernova. Far above in energy scale and 56Ni production lies SN 1998bw, the only supernova firmly associated with a gamma-ray burst.
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Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
A population synthesis study with a hybrid TIDE+L dynamical model predicts that the Cherenkov Telescope Array Observatory will detect roughly ten times more Galactic pulsar wind nebulae than are currently known in TeV gamma rays.