Researchers found 'anomalous X-ray pulsars' in supernovae remnants, which spin slower and have stronger magnetic fields than radio pulsars. This discovery reverses the understanding of how pulsars behave after a star explodes as a supernova.
Astronomers detect powerful gamma rays from SGR 1900+14, confirming the existence of magnetars and linking three mysteries: what are Soft Gamma Repeaters (SGRs) and Anomalous X-ray Pulsars (AXPs)? The discovery provides insights into neutron star behavior and suggests a million old magnetars might be drifting through the Galaxy
Astronomers Renyue Cen suggests that gamma-ray bursts might come from supernovae expelling material at high speeds, producing jets that travel at nearly the speed of light. This theory could explain why some pulsars are moving faster than ordinary stars and potentially pose a catastrophic threat to Earth.
A rapidly spinning neutron star, SAX J1808.4-3658, is providing proof for the theory that millisecond pulsars are propelled to mind-boggling speeds by accretion of material from a companion star. This discovery fills an important niche in our understanding of star evolution.
Astronomers detected a series of at least 26 starquakes, leading to the discovery of SGR 1627-41, the fourth conclusively identified SGR. The new SGR is believed to be caused by massive starquakes and has been linked to a supernova remnant.
Researchers measured the velocity of gases ejected during an early phase of supernova formation, allowing them to tie its formation to the star's evolutionary phases. The study found that the entire nebula is at least 200,000 years old and probably several times older.
Researchers studied 40 distant supernovae to measure the cosmic expansion rate, finding it will expand forever due to insufficient mass for gravity to slow it down. Type Ia supernovae provide natural mile-markers to track trends in the universe's expansion.
Astronomers calculate that a gamma ray burst has expanded to 85 times the size of our solar system and is still growing. The detection uses the 'twinkling' effect in radio astronomy, where the point where twinkling stops allows for diameter measurement.
New observations reveal DEM L 316 as two overlapping supernova remnants with colliding shells, studied to understand energy and element distribution. The collision may influence the births of new stars by distributing material from dead stars.
Astronomers predict that the debris cloud from Supernova 1987A will continue to expand and brighten over the next decade, reaching its final stage by 2007 A.D. The ring of hydrogen gas surrounding the supernova is expected to increase in brightness by a factor of 1,000.
The Katzman Automatic Imaging Telescope (KAIT) is a fully robotic telescope that can track a given area of the sky for hours and detect objects 10,000 times fainter than other telescopes. KAIT will enable astronomers to conduct nightly studies of changing celestial objects remotely.
Researchers at Oak Ridge National Laboratory will study nuclei in stellar explosions and exotic nuclear structures, answering questions about nuclear physics and astrophysics. The facility provides a resource for scientists from around the world, offering insights into the main constituent of the visible universe.