| Integral has a large field of view, enabling it to scan our Milky Way galaxy for neutron stars and black hole activity. |
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| This process also stabilizes white dwarfs and neutron stars against gravitational collapse. |
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| Stellar remnants such as white dwarfs, neutron stars, and black holes will remain. |
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| That kind of resolution is good for small objects like neutron stars, gamma ray bursts and black holes. |
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| This means that neutron stars are formidable radiation emitters and particle accelerators. |
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| These sources have been attributed to white dwarfs, neutron stars and black holes. |
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| However, most neutron stars have a mass of about 1.35 solar masses, albeit with interesting exceptions. |
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| Stars with a smaller amount of mass evolve into less compressed bodies, either white dwarfs or neutron stars. |
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| Giacconi, who shared the 2002 Nobel Prize for Physics, was on his way to showing that neutron stars could be bound in binary systems along with normal stars. |
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| Most neutron stars are created when a large star dies as a supernova. |
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| The stars are replaced by a homogenous sea of glowing hot gas with embedded jewels of stellar accretion disks, neutron stars and super nova remnants. |
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| It also predicted neutron stars and black holes, although they weren't accepted for many decades. |
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| Colliding neutron stars was a popular one for a while, but fell out of favour. |
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| The pulsars, of which more than one thousand are known today, are interpreted as being neutron stars in rotation. |
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| The most recent detection, this fall, recorded the disruption caused by merging neutron stars. |
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| Many dying stars collapse to become cosmic exotica like black holes or neutron stars. |
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| A small fraction of the absent mass might be mundane: sunless planets, wandering black holes, neutron stars and the like. |
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| The U. S. space agency NASA is among the research and exploration agencies interested in Vicky Kaspi's work on pulsars and other neutron stars. |
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| Pulsars are identified with strongly magnetized, rapidly-rotating neutron stars. |
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| For that reason, such objects are called pulsars, and they have provided our best data about neutron stars. |
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| These objects are now known to be neutron stars, the collapsed cores of massive stars that have ended their lives in vast outbursts known as supernova explosions. |
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| Could they be red giant stars, white dwarfs, or neutron stars? |
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| Experts on very compact white dwarfs, neutron stars, and black holes study the enormously energetic and fascinatingly rich array of phenomena that these systems exhibit. |
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| They successfully matched the orbital behaviour of the two neutron stars with the behaviour predicted according to Einstein's theory. |
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| Success in finding an object that had previously been too difficult to detect suggests that even faster spinning neutron stars likely exist. |
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| Such an area of instability, bounded by the last stable orbit, exists around neutron stars in slow rotation. |
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| It includes neutron stars and black holes, natural plant products, and Aristotelian philosophy. |
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| Or they could be from point sources, mainly black holes and neutron stars. |
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| Astronomers suspect they are linked with imploding neutron stars or eruptions on magnetars. |
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| The researchers compared this mass with predictions in various computer models and determined that zinc-82 is probably absent from neutron stars. |
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| He and his German colleague did it by simulating what happens when dense neutron stars spiral together and collide in deep space. |
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| Pulsars are rapidly spinning neutron stars, the superdense remains of massive stars that have exploded as supernovas. |
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| In 1974, the discovery of a binary pulsar-a pair of neutron stars that rotate around each other-provided unique conditions to test relativity more thoroughly. |
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| When these neutron stars merge with others in the center of our galaxy, they could produce a gamma ray burst that would greatly affect the galaxy. |
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| The discovery of the most rapidly rotating neutron star ever found challenged earlier models that had suggested it was not possible for neutron stars to spin so fast. |
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| A significant qualitative difference found between strange and neutron stars is that, outside strange stars, there is a last stable orbit even for high disk speeds. |
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| In fact, in certain extreme environments, such as neutron stars, extreme temperature and pressure prevents atoms from existing at all. |
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| The discovery of neutron stars sparked interest in gravitationally collapsed compact objects as a possible astrophysical reality. |
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| Such observations can be used to exclude possible alternatives such as neutron stars. |
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| This process was helped by the discovery of pulsars in 1967, which, by 1969, were shown to be rapidly rotating neutron stars. |
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| Other compact objects, such as neutron stars, can also have photon spheres. |
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| This occurs in environments with a high neutron density, such as a supernova or the merger of two neutron stars. |
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| Starquakes in slowing neutron stars drive matter toward the magnetic poles, distort the star's shape, and excite precession. |
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| This is surprising, and that much mass means that several theoretical models for the internal composition of neutron stars now are ruled out. |
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| According to this theory, this magnetic funneling happens in the same way on all neutron stars and all hot spots should be about the same size. |
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| It provided the first solid evidence that neutron stars exist. |
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| The accumulation of such observations will undoubtedly make it possible to differentiate neutron stars from strange stars, which will have significant repercussions for the physics of the matter at very high density. |
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| I think of these neutron stars as the last stop before black holes. |
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| He is speaking about stars such as hot white dwarfs and neutron stars, black holes and quasars that are seen principally in UV and X-ray wavelengths. |
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| Black holes, neutron stars, pulsars, white dwarfs, quasars, and active galactic nuclei are just some of the cosmic objects that ASTROSAT will offer a glimpse of. |
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| It is one of about two dozen neutron stars called magnetars, which have very powerful magnetic fields and occasionally produce high-energy explosions or pulses. |
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| The precise measurement of an exotic atom in the laboratory has refined scientists' understanding of neutron stars, which are among the universe's most extreme objects. |
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| There, he had used radio waves to probe the secrets of pulsars, the spinning, magnetized neutron stars that emit bursts of radiation with clocklike regularity. |
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| Explaining a theory on the radio burst causes, study co-author Matthew Bailes said they are likely the result of neutron stars, also known as magnetars. |
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| Thorne-Zytkow objects are hybrids of red supergiant and neutron stars that superficially resemble normal red supergiants, such as Betelguese in the constellation Orion. |
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| Astronomers have measured an effect long predicted by Einstein's theory of General Relativity in the extremely strong gravity of a pair of superdense neutron stars. |
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| Neutron stars in binary star systems, however, can reverse this trend and speed up with the help from the companion star. |
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| Neutron stars such as IGR J16283-4838 are often part of binary systems, orbiting a normal star. |
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| Neutron stars are the most dense objects of normal matter in the universe, supported against gravitational collapse by subatomic forces. |
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| Neutron stars are too far away for astronomers to study their composition, and scientists cannot re-create their enormous pressures in the lab. |
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| Neutron stars are extremely compact objects, resulting from supernova explosions of dying massive stars with 8 to 20 solar masses. |
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