Explanation: As far as pulsars go, PSR B1509-58 appears young. Light from the supernova explosion that gave birth to it would have first reached Earth some 1,700 years ago. The magnetized, 20 kilometer-diameter neutron star spins 7 times per second, a cosmic dynamo that powers a wind of charged particles. The energetic wind creates the surrounding nebula's X-ray glow in this tantalizing image from the Chandra X-ray Observatory. Low energy X-rays are in red, medium energies in green, and high energies in blue. The pulsar itself is in the bright central region. Remarkably, the nebula's tantalizing, complicated structure resembles a hand. PSR B1509-58 is about 17,000 light-years away in the southern constellation Circinus. At that distance the Chandra image spans 100 light-years.
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Publikacii s klyuchevymi slovami:
pulsar - neutron star - Pul'sar - neitronnye zvezdy - rentgen - rentgenovskie luchi - Rentgenovskii pul'sar
Publikacii so slovami: pulsar - neutron star - Pul'sar - neitronnye zvezdy - rentgen - rentgenovskie luchi - Rentgenovskii pul'sar | |
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