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The propagation of high-energy cosmic rays through giant molecular clouds constitutes a fundamental process in astronomy and astrophysics. The diffusion of cosmic-rays through these magnetically turbu...
The propagation of high-energy cosmic rays through giant molecular clouds constitutes a fundamental process in astronomy and astrophysics. The diffusion of cosmic-rays through these magnetically turbu...
Askaryan Radio Array (ARA), a large-scale radio Cherenkov observatory which scientists propose to develop in Antarctica, aims at discovering the origin and evolution of the cosmic accelerators that pr...
The BOOTES experiment in support of the Gran Telescopio Canarias (GTC) in the study of the high energy Universe。
Ultra-high-energy cosmic ray acceleration by magnetic reconnection in newborn pulsars。
Very High Energy Gamma-rays from Galactic Sources     ray astronomy  PACT       font style='font-size:12px;'> 2009/5/19
The field of Very High Energy (VHE) gamma ray astronomy using the Atmospheric Cerenkov Technique has entered an interesting phase with detection of various galactic and extragalactic sources. Among ...
High Energy Phenomena in Eta Carinae     non-thermal emission stars  Car—X-ray emission       font style='font-size:12px;'> 2009/5/19
We have investigated with BeppoSAX the long term behaviour of the harder X-ray component of the supposed supermassive binary system  Car along its 5.52 year cycle. We have found that in March 1998 ...
The average characteristics of the diurnal and semi-diurnal anisotropy of cosmic ray intensity at relativistic energies have been obtained by using data from the worldwide grid of neutron monitor fo...

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