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The Crab Nebula (also designated M1 or NGC 1952) is visible through small telescopes, which has allowed astronomers to observe its growth and evolution since the supernovae that created it became visible in 1054 CE. A pulsar was found in the center of the Crab in 1968. This rapidly rotating neutron star is the core of the star that went supernova to make the nebula. In the intervening decades, X-ray, gamma ray, and radio observations have mapped the region of the nebula closest to the pulsar. During that mapping, it became apparent that the Crab pulsar is one of the brightest sources of gamma rays observable from Earth. Despite all of those observations, we still don't fully understand the Crab's precise gamma ray spectrum, particularly recently observed pulses of intense gamma radiation seen by the Fermi Gamma-ray Space Telescope. Existing models certainly do well at describing much of the complex interplay between the intense magnetic fields of the pulsar and the winds of charged...

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Communications, Engineering & Design Magazine NewNet sees WiMax opportunities in Canada ITWorld Canada A US-based wireless equipment company that has expanded into WiMax solutions says there are opportunities north of the border to sell the systems, despite falling North American demand for the technology. Officials at NewNet Communications Technologies ... NewNet sees opportunity in WiMAXCommunications, Engineering & Design Magazine all 3 news articles »