Articles tagged with Supernovae
The ESO team has provided conclusive evidence linking cosmological gamma-ray bursts to hypernova explosions, suggesting a direct connection between the two events. The study uses unprecedented spectral data from the VLT KUEYEN telescope to determine the distance of the burst as approximately 2,650 million light-years.
Recent RHESSI detection suggests gamma-ray bursts originate from highly structured magnetic fields, stronger than neutron star surfaces. This finding implies a dramatic shift in understanding the physics behind these explosive events.
A new 3D map of local space reveals the Sun at the center of an irregular cavity, surrounded by a dense wall of gas. The map suggests that interlocking cavities and tunnels were created by supernovas or strong stellar winds.
The Nearby Supernova Factory has achieved its best rookie year due to the high-speed link provided by the High Performance Wireless Research and Education Network (HPWREN). This allows for rapid image processing and analysis, leading to a higher number of discovered supernovae. The project's success demonstrates the benefits of partner...
Researchers observed supernova remnants in two neighboring galaxies, providing new insight into gas shocked by blast waves and material structure between stars. The findings expand our understanding of a star's long-term evolution and how elements are redistributed into interstellar space.
Lawrence Livermore physicist Bruce Remington explores using lab astrophysics to recreate supernovae explosions, understand cosmic rays, and study black holes. Lab experiments also aim to probe planet interiors and gamma-ray bursts.
A new theory suggests that an ancient supernova explosion may have devastated the Earth's ocean ecosystem, causing widespread extinction of plankton and marine organisms. The discovery was made by linking data from paleontology, geology, and astronomy fields.
The TIGER experiment is making a groundbreaking second loop around the South Pole to study the origin of cosmic rays. By examining abundance ratios of neighboring elements, scientists aim to determine whether atoms were accelerated individually or as dust grains, and gain insights into supernovas.
Researchers using NASA's Chandra X-ray Observatory have discovered a probable pulsar at the center of a 1,600-year-old supernova. The finding provides evidence for an associated pulsar and allows for detailed study of the supernova remnant. This discovery helps connect pulsars with massive stars from which they formed.
A team of Belgian and French astronomers have discovered three distant stars with extremely high Lead abundances, exceeding other elements heavier than Iron. This finding aligns with current stellar models predicting the buildup of heavy elements in stellar interiors.
Researchers will model and study supernovae to discover how they occur and the complex physical processes involved. They aim to understand challenging issues in theoretical and computational physics, advancing national security interests.
Researchers create method to determine subatomic particle mass based on speed of material streaming from a supernova, which could improve nuclear reaction understanding and dark matter detection. The technique hinges on the formation of black holes in about half of observed supernovas, allowing for precise timing of neutrino arrival.
Dr. Oliver Manuel proposes that the sun and planets formed from debris of a massive supernova explosion, contradicting conventional astrophysics theories. Recent data from NASA's Galileo probe supports his claims by detecting traces of strange xenon gases in Jupiter's atmosphere.
Researchers suggest that a rare radioactive isotope found in deep-sea sediments may be evidence of a nearby supernova. The explosion could have caused a 'cosmic-ray winter' leading to mini-extinctions about 5 million years ago, with effects still detectable today.
The Hobby-Eberly Telescope has successfully observed a distant quasar candidate, confirming its status and providing insight into the universe's early evolution. The instrument will also enable detailed study of objects in and near the Milky Way with the addition of two new facility-class spectrographs.
A new chemical sequence has been uncovered, casting doubt on long-held equilibrium theory and clearing the way for kinetic chemistry. The finding breaks the strong bond between carbon and oxygen atoms under intense radioactivity conditions.
Researchers found supernovas are fainter than expected, suggesting the universe has expanded more slowly in the past and is now accelerating. This discovery supports the Cosmological Constant theory, which had been dismissed by Albert Einstein, and has significant implications for our understanding of the universe's behavior.
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.
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.
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.