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You entered: neutron
![NGC 4697: рентгеновское излучение из эллиптической галактики](https://images.astronet.ru/pubd/2002/06/17/0001177380/ngc4697_cxc_c1.preview.jpg)
17.06.2002
The many bright, point-like sources in this Chandra Observatory x-ray image lie within NGC 4697, an elliptical galaxy some 40 million light-years away towards Virgo. Like other normal elliptical galaxies, NGC 4697 is a spherical ensemble of mainly older, fainter, low mass stars, with little star forming gas and dust compared to spiral galaxies.
![GW170817: регистрация излучения разных видов от явления слияния](https://images.astronet.ru/pubd/2017/10/16/0001390709/ns.preview.jpg)
16.10.2017
Both gravitational and electromagnetic radiations have been detected in rapid succession for an explosive merging event for the first time. Data from the outburst fit well with a spectacular binary neutron-star death-spiral. The explosive episode was seen on August 17 in nearby NGC 4993, an elliptical galaxy only 130 million light years distant.
![N44C: загадочная туманность](https://images.astronet.ru/pubd/2002/05/14/0001176788/n44c_hst.preview.jpg)
14.05.2002
Why is N44C glowing so strangely? The star that appears to powers the nebula, although young and bright, does not seem hot enough to create some of the colors observed. A search for a hidden hotter star in X-rays has come up empty.
![Пульсар и движение газа в Крабовидной туманности](https://images.astronet.ru/pubd/2002/09/20/0001179815/crabshrug_rox_big.preview.jpg)
20.09.2002
How does a city-sized neutron star power the vast Crab Nebula? The expulsion of wisps of hot gas at high speeds appears to be at least part of the answer. Yesterday time-lapse movies taken...
![Остаток сверхновой CTA 1](https://images.astronet.ru/pubd/2024/08/23/0001936047/CTA1_15_75_Lelu1024.preview.jpg)
23.08.2024
There is a quiet pulsar at the heart of CTA 1. The supernova remnant was discovered as a source of emission at radio wavelengths by astronomers in 1960 and since identified as the result of the death explosion of a massive star.
![Рентгеновский пульсар](https://images.astronet.ru/pubd/2003/12/10/0001195541/millisec_pulsar_big.preview.jpg)
23.07.1998
This dramatic artist's vision shows a city-sized neutron star centered in a disk of hot plasma drawn from its enfeebled red companion star. Ravenously accreting material from the disk, the neutron star spins faster and faster emitting powerful particle beams and pulses of X-rays as it rotates 400 times a second.
![APOD: 2024 July 23 Б The Crab Nebula from Visible to X Ray](https://images.astronet.ru/pubd/2024/07/23/0001934003/Crab_MultiChandra_960.preview.jpg)
23.07.2024
What powers the Crab Nebula? A city-sized magnetized neutron star spinning around 30 times a second. Known as the Crab Pulsar, it is the bright spot in the center of the gaseous swirl at the nebula's core.
![Сверхновая выстреливает пульсар J0002](https://images.astronet.ru/pubd/2019/08/13/0001490727/CannonSupernova_English_960.preview.jpg)
13.08.2019
What could shoot out a neutron star like a cannon ball? A supernova. About 10,000 years ago, the supernova that created the nebular remnant CTB 1 not only destroyed a massive star but blasted its newly formed neutron star core -- a pulsar -- out into the Milky Way Galaxy.
![Сверхновая выстреливает пульсар J0002](https://images.astronet.ru/pubd/2022/10/02/0001850427/CannonSupernova_English_960.preview.jpg)
2.10.2022
What could shoot out a neutron star like a cannon ball? A supernova. About 10,000 years ago, the supernova that created the nebular remnant CTB 1 not only destroyed a massive star but blasted its newly formed neutron star core -- a pulsar -- out into the Milky Way Galaxy.
![Магнетар на небе](https://images.astronet.ru/pubd/2004/11/27/0001201304/magnetarcobe.preview.jpg)
2.10.1998
Indicated on this infrared image of the galactic center region is the position of SGR 1900+14 - the strongest known magnet in the galaxy. SGR 1900+14 is believed to be a city-sized, spinning, super-magnetic neutron star, or Magnetar. How strong is a Magnetar's magnetic field?
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