Neutrinos provide new route to heavy elements in supernovae
During their long lifetimes stars generate their energies by nuclear fusion in their interiors, which are generally accepted to be the breeding grounds for carbon and heavier elements.
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During their long lifetimes stars generate their energies by nuclear fusion in their interiors, which are generally accepted to be the breeding grounds for carbon and heavier elements.
Observations of very high-energy gamma-rays from two distant active galaxies reveal that the universe is more transparent to this radiation than previously thought. This limited absorption of gamma-ra...
Almost every current theoretical model of neutrino masses introduces sterile ("right-handed") fields, which mix with the ordinary ("left-handed") neutrinos.
NASA’s Wilkinson Microwave Anisotropy Probe (WMAP) collaboration has finally released new observations of cosmic microwave background (CMB) radiation with updated results on the nature and origi...
James Pinfold reports on the large number of projects that are forging a connection between research in ultra-high-energy cosmic rays and practical scientific experience in schools.
Antonella del Rosso reviews (in French) in 2006 300 questions à un astronome.
Roger Anthoine reviews (in French) in 2006 Quand le Ciel nous bombarde: Qu'est-ce que les rayons cosmiques?
An international team of astronomers using the Parkes radio telescope in Australia has detected very short radio flashes from 11 sources distributed in the plane of our galaxy. The isolated flash...
The C2CR meeting in Prague targeted the interface between cosmic-ray physics and the current and future results from accelerators and colliders.
A planet of a mass of only about five times that of the Earth has been discovered at a distance of about 20,000 light years, not far from the centre of the Milky Way. It circles its parent low-mass st...