Articles tagged with Gamma Ray Bursts
A team of astronomers suggests that Type Ic supernovae could produce gamma-ray bursts through the collapsar model, which proposes an asymmetric explosion mechanism and a jet of particles and energy. The theory is supported by observations with Keck and Subaru telescopes in Hawaii.
Astronomers have detected a unique visible light component that varies with gamma rays, suggesting a common origin for both. This finding contradicts previous theories and sheds new light on the nature of these powerful cosmic events.
The NASA-led Swift mission has successfully measured the distances to two gamma-ray bursts, both originating from over 9 billion light years away. These direct distance measurements, achieved with Swift's Ultraviolet/OpticalTelescope (UVOT), represent a major milestone for the mission since its launch in 2004.
The Swift satellite's Ultraviolet/Optical Telescope (UVOT) has captured an image of the Pinwheel Galaxy, revealing regions of star formation in the galaxy's spiral arms. The UVOT will also help scientists determine the distance to closer gamma-ray bursts and study their afterglows.
The Swift X-ray Telescope has successfully captured its first gamma-ray burst afterglow, marking a significant milestone in the mission to understand these mysterious events. The telescope will help scientists pinpoint the location and nature of the explosion, providing crucial clues about the origins of gamma-ray bursts.
The Swift satellite will pinpoint the location of distant gamma-ray bursts, studying both the burst and its afterglow. It may uncover new clues about the burst mechanism and provide a bonanza of cosmological data, including information about supermassive black holes.
The study reveals that strong magnetic fields accelerate particles near the speed of light, radiating as gamma rays. The research suggests a new mechanism for gamma-ray burst formation, potentially resolving long-standing scientific debates.
Astronomers have discovered two unique rings of dust illuminated by the afterglow of a gamma-ray burst in our galaxy. The rings, caused by dust scattering X-rays from the burst, reveal new insights into the distribution and behavior of dust in the Galaxy.
A team of astronomers studied the polarisation properties of GRB 030329's afterglow over 38 days, detecting significant variability in strength and orientation. The data reveal a unique diagnostic tool for gamma-ray burst studies, challenging existing theories.
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.
The gamma ray burst, discovered by the ROTSE (Robotic Optical Transient Search Experiment) collaboration, has an intensity 100 times greater than previously observed. Its proximity to Earth allows for detailed study of its decaying light.
Researchers found a correlation between fluence and duration for both short and long bursts, but the degree of this relationship is statistically different at a 4.5 sigma significance level. This suggests that short bursts may originate from fundamentally different physical processes than long bursts.
The University of California, Berkeley's robotic telescope has captured the earliest image of a gamma-ray burst's optical afterglow, offering unprecedented data for theorists to study. The data provides key constraints for physical models of gamma-ray bursts and will help astronomers better understand these enigmatic events.
A new MIT model proposes that cosmic explosions may be triggered by a cosmic tango between a black hole and its companion, a spinning torus of stellar material. The model suggests that the energy released during this dance could explain recent observations of gamma-ray bursts.
Rice University researchers have developed a new technique to calculate the distance of gamma-ray bursts, enabling scientists to learn more about the early universe's formation and evolution. The method uses changes in color to determine the cooling rate of high-energy pulses in these cosmic events.
Neutrinos may fly out first in powerful gamma-ray bursts, carrying details of the universe's first stars. Scientists believe neutrino bursts can help detect massive star collapses and dark gamma-ray dark collapses.
Researchers found evidence that supernovae explosions can leave behind iron-rich gas clouds that feed gamma-ray bursts. The 'supranova' model suggests that the gamma-ray burst arises from the delayed collapse of a neutron star formed by the supernova explosion.
The Interplanetary Network detected a gigantic gamma-ray burst, the most distant ever observed, from a dying star 30 times more massive than the sun. The burst is believed to have occurred 11 billion years ago and has been traveling through space for the same amount of time.
A team led by Dr. Charles Meegan is developing a new burst monitor to fly on the Gamma Ray Large Area Space Telescope, which will provide broad energy coverage for gamma-ray studies and help solve the nature of gamma-ray bursts.
Compton Gamma Ray Observatory's Burst And Transient Source Experiment (BATSE) discovered nearly 30 new exotic astrophysical objects and phenomena, rewriting astronomy textbooks. The instrument also contributed to 10 scientific prizes and 18 Ph.Ds.
Astronomers pinpointed a gamma-ray burst's precise location using coordinated observations from NASA satellites, providing data on X-rays and visible energy. The blast occurred over 10 billion light years away, roughly 2 billion years after the Big Bang.
Astrophysicists use 'forensic science' to study gamma-ray bursts, seeking clues about their causes. Observations suggest that many bursts are linked to star formation and blue galaxies.
Gamma-ray bursts remain a mystery despite over 2,500 recorded events and numerous burst sources identified. Scientists caution against interpreting data carefully due to potential systematic errors in measurement systems.
Researchers discuss alternative theories for Magnetar outbursts, including the role of intense magnetic fields and environmental influences. The magnetar theory suggests that giant flare events occur when the neutron crust cracks, while an alternative explanation proposes a relativistic wind of interstellar material surrounding the SGR.
Astronomers have found evidence of a prompt high-energy afterglow component from a gamma-ray burst, suggesting multiple energy emission processes and mechanisms. This discovery supports the idea that different activities cause what appears to be a chaotic explosion.
A gamma-ray burst may have melted primordial dust grains, seeding the formation of meteorites and rocky planets like Earth. The theory suggests that only one Sun-like star in a thousand would be close enough to form chondrules.
The 'braking glitch' in the spin rate of a soft gamma repeater (SGR) suggests a massive starquake may have occurred. The SGR's rotational period increased steadily until a rapid decrease was observed, indicating a massive energy release.
Dr. Colleen Wilson-Hodge, a NASA astrophysicist, has discovered two new X-ray pulsars using the Burst and Transient Source Experiment on NASA's Compton Gamma Ray Observatory. The pulsars are powered by accretion of material from companion stars and have strong gravity that pulls matter toward their surfaces.
Researchers use telescopes and computer simulations to understand gamma-ray burst explosions. They find evidence of shock waves generated by collisions between material flowing out at different velocities, potentially revealing the cause of initial visible light emission.
Astronomers have detected the brightest optical celestial object ever recorded using a low-cost, automated telescope built from recycled lenses and hardware. The ROTSE-1 telescope captured optical emissions from a gamma ray burst while it was still arriving, providing new insights into the phenomenon.
Astrophysicist James Annis suggests that cataclysmic gamma-ray bursts could be sterilizing galaxies, preventing extraterrestrial life from reaching Earth. This theory may provide an explanation for the Fermi Paradox, with intelligent life having recently emerged in the Galaxy and being unable to explore yet.
A new pulsar has been discovered orbiting a massive star, providing insights into the mysterious behavior of transient objects. The pulsar, named XTE J1946+274 or GRO J1944+26, exhibits complex orbital patterns and intense magnetic fields, challenging our understanding of these enigmatic celestial bodies.
A rapidly spinning neutron star can naturally produce a Gamma-ray burst by oscillating and radiating its rotation energy. The spin-down process is triggered by the gravitational wave instability, which grows explosively in hours or minutes, strengthening the magnetic field and eventually radiating away all remaining rotation energy.
Recent study examines over 100 gamma-ray bursts, finds no evidence supporting synchrotron shock model. Researchers analyze low-energy spectra to determine burst causes.
A powerful gamma-ray and X-ray burst from a distant star caused significant changes in Earth's upper atmosphere, leading to increased ionization levels and reduced radio signal range. The event has implications for our understanding of the ionosphere and its interactions with external energy sources.
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 propose instrument to measure high-energy gamma rays from blazars, pulsars, and bursts, offering improved tracking capabilities and higher energy detection limits. The scintillating fiber detector system will act as both a tracker and calorimeter, providing a wide-angle view of the sky with unprecedented precision.
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.
Scientists are making significant progress in discovering gamma-ray burst counterparts and afterglows, shedding light on these mysterious events. Fourteen papers are scheduled to be presented at the session, covering the electromagnetic spectrum from radio to gamma rays.
Recent discoveries have revealed that Gamma-Ray Bursts originate from the most remote parts of the universe, releasing enormous amounts of energy in just 10 seconds. The high-redshift burst announcement adds to the body of research indicating these explosions are the most powerful in the Universe.
Scientists at Columbia University detected the largest explosion ever witnessed, a gamma-ray burst, which occurred 12 billion years ago. The event released almost as much energy as the 10 billion trillion stars in the universe combined and was detected using a rapid series of phone calls between astronomers around the world.
A NASA scientist has found a new puzzle in the sky, an X-ray pulsar that appears to burst twice every 'year' rather than once. Colleen Wilson discovered GRO J2058+42, which has no visible component and exhibits unusual behavior, suggesting it may be a binary star system with a type Be star and a neutron star in a lopsided orbit.
Astrophysicists have solved a decades-old mystery with the identification of gamma-ray burst counterparts, leading to a deeper understanding of the universe's early stages. Dr. Jan van Paradijs' discovery of an optical counterpart for a gamma-ray burst in 1997 marked a significant breakthrough.
The 191st AAS meeting will feature a lecture on the latest research on gamma-ray bursts, revealing their origin from distant reaches of the universe. Dr. Chryssa Kouveliotou and Sir Martin Rees will present new findings on GRB characteristics, including temporal, spectral, and spatial analysis.
NASA's Burst and Transient Source Experiment (BATSE) has recorded its 2000th gamma-ray burst, a significant milestone in the study of these violent cosmic events. The 2000th burst was smaller than average, but adds to the growing body of knowledge about gamma rays and their origins.
The Johns Hopkins University Applied Physics Laboratory's NEAR spacecraft has detected a major gamma-ray burst, validating its instrument as a true partner in the interplanetary network. The detection expands the network to locate gamma-ray sources with greater accuracy.
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.
Despite intensive searches, only a few gamma ray burst counterparts have been found, leaving scientists with more questions than answers. The lack of consistent patterns hampers the search, but continued observations with powerful instruments may help clarify the issue.
Scientists have discovered that the May 8 gamma ray burst releases an enormous amount of energy, outshining the sun in its lifetime. Radio observations indicate the fireball expands at nearly the speed of light, with a size estimated to be about one-tenth of a light-year.
Recent discoveries demonstrate that Gamma-Ray Bursts (GRBs) originate from the most remote parts of the universe, releasing as much energy in 10 seconds as the Sun emits in its entire lifetime. The uniform distribution on the sky and brightness distribution rule out galactic halo and suggest distances exceeding billions of light years.
Astronomers have detected radio emission from a cosmic gamma-ray burst using the National Science Foundation's Very Large Array (VLA) radio telescope. The detection may help resolve one of the biggest mysteries in astrophysics, providing unprecedented knowledge about gamma-ray bursts and their parent objects.
A team of astrophysicists discovered fewer low-energy photons in the universe than previously thought, suggesting that high-energy gamma rays may not be interacting with as many low-energy photons as expected. This observation could alter current theories of the history of the universe and galaxy formation.
Astronomers have detected a flash of light from a distant galaxy, potentially solving a 30-year mystery in astrophysics. The discovery suggests gamma-ray bursts originate from the distant reaches of the universe.
Astronomers analyze over 1,700 gamma-ray bursts and find they are isotropic, meaning their distribution on the sky is almost perfectly random. This contradicts previous theories that placed these bursts within or just outside of our own Milky Way Galaxy.
Astronomers use BATSE to detect four rare cosmic gamma-ray bursts, sparking debate about their origin and distance. The events appeared in rapid succession over two days from the same general position in the sky.
The Compton Observatory detected the brightest gamma-ray burst in its five and a half year mission, releasing as much energy in tens of seconds as the Sun will produce in ten-billion-year lifetime. The burst is rare and may contain information about sources that cannot be extracted from weaker events.
A team of astronomers observed extremely rapid bursts of high-energy gamma rays from a distant galaxy, challenging current theoretical models. The bursts were extremely rapid, occurring in under half an hour, while previous flares occurred over days or minutes.