supernova remnant oor Noorse Bokmål
supernova remnant
en
(astronomy) A nebula that is formed from supernova explosion debris.
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supernovarest
en
remnants of an exploded star
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Supernova remnant: Radio image in red, X-ray in blue, visible light in green
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I've narrowed it down to the MacPherson Nebula, a supernova remnant, and Dikon Alpha, a class-nine pulsar.
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Other objects commonly observed in ultraviolet light include planetary nebulae, supernova remnants, and active galactic nuclei.
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Notable X-ray sources include X-ray binaries, pulsars, supernova remnants, elliptical galaxies, clusters of galaxies, and active galactic nuclei.
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The former deals with objects such as the galaxies of the Local Group, which are close enough to allow very detailed analyses of their contents (e.g. supernova remnants, stellar associations).
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Astronomers, such as Harvard’s Robert Kirshner, believe that understanding supernova remnants like the Crab Nebula is important because they can be used to measure the distance to other galaxies, which is currently an area of intense research.
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It's a remnant of a supernova.
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These massive stars produce supernova explosions, resulting in expanding remnants that interact powerfully with the surrounding gas.
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The Vela supernova remnant is an expanding shell of gas that originated from the supernova explosion.
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Each of these four fabulous photographs shows the remains of an exploded star — called a supernova remnant.
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The Key elements of life, such as phosphorus, according to the results of 2013, was discovered in supernova remnants.
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These pulsar planets are thought to have formed from the unusual remnants of the supernova that produced the pulsar, in a second round of planet formation, or else to be the remaining rocky cores of gas giants that somehow survived the supernova and then decayed into their current orbits.
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This space photograph shows a 2200-year-old supernova remnant that is sweeping up a remarkable amount of material — enough to make 45 Suns!
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This is the Vela supernova remnant, gas clouds that were ejected from a dying star in a huge explosion about 11 000 years ago.
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The image on the left shows the entire SN 1006 supernova remnant, as seen in radio (red), X-ray (blue) and visible light (yellow).
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The study was the first to use an integral field spectrograph [3] to probe the properties of the shock fronts of supernova remnants in such detail.
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For the first time the observations suggest the presence of fast-moving particles in the supernova remnant that could be the precursors of such cosmic rays.
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We pass many interesting objects, including star formation regions and the blue filaments of a supernova remnant, before closing in on the faint star IRAS 08544-4431.
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The associated supernova remnant is a characteristic cloud of gas blown away by the shock wave resulting from the collapse of the star into a neutron star.
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From this ideal position Chandra can create X-ray pictures with superb detail, allowing us to study the shape, movement and chemical make-up of supernova remnants.
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"The new ALMA results, which are the first of their kind, reveal a supernova remnant chock full of material that simply did not exist a few decades ago."
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They had dense, dark, dusty heads and long, faint tails, which were generally pointing away from the Vela supernova remnant located at the centre of the Gum Nebula.
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Supernova remnants don’t actually create any energy of their own, meaning their supply will eventually run out and each of these beautiful objects will fade away until they’re invisible.
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After a short lifetime of about ten million years, the massive companion would have exploded as a supernova — which could explain the characteristic gas cloud known as a supernova remnant found nearby.
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It has long been suspected that such supernova remnants may also be where some cosmic rays — very high energy particles originating outside the Solar System and travelling at close to the speed of light — are formed.
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41 sinne gevind in 11 ms. Hulle kom uit baie bronne en word nie nagegaan nie.