File:Astronomers Find the First 'Wind Nebula' Around a Rare Ultra-Magnetic Neutron Star (27744663791).jpg

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English: Astronomers have discovered a vast cloud of high-energy particles called a wind nebula around a rare ultra-magnetic neutron star, or magnetar, for the first time. The find offers a unique window into the properties, environment and outburst history of magnetars, which are the strongest magnets in the universe.

A neutron star is the crushed core of a massive star that ran out of fuel, collapsed under its own weight, and exploded as a supernova. Each one compresses the equivalent mass of half a million Earths into a ball just 12 miles (20 kilometers) across, or about the length of New York's Manhattan Island. Neutron stars are most commonly found as pulsars, which produce radio, visible light, X-rays and gamma rays at various locations in their surrounding magnetic fields. When a pulsar spins these regions in our direction, astronomers detect pulses of emission, hence the name.

This X-ray image shows extended emission around a source known as Swift J1834.9-0846, a rare ultra-magnetic neutron star called a magnetar. The glow arises from a cloud of fast-moving particles produced by the neutron star and corralled around it. Color indicates X-ray energies, with 2-3 KeV in red, 3-4.5 keV in green, and 5-10 keV in blue. The image combines observations by the European Space Agency's XMM-Newton spacecraft taken on March 16 and Oct. 16, 2014.
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Source https://www.nasa.gov/image-feature/goddard/2016/first-wind-nebula-around-a-magnetar
Author ESA/XMM-Newton/Younes et al. 2016
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https://xmm-tools.cosmos.esa.int/external/xmm_science/gallery/public/level3.php?id=1223

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Attribution: ESA/XMM-Newton/Younes et al. 2016, CC BY-SA IGO 3.0
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current08:44, 2 July 2017Thumbnail for version as of 08:44, 2 July 20171,920 × 1,086 (457 KB)Huntster (talk | contribs)Larger file.
19:49, 17 September 2016Thumbnail for version as of 19:49, 17 September 20161,041 × 589 (36 KB)Vanished Account Byeznhpyxeuztibuo (talk | contribs)Transferred from Flickr via Flickr2Commons

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