Articles tagged with Gamma Ray Astronomy
Researchers have located the site of relativistic particle acceleration in galaxy M 87, where particles are accelerated to extreme energies and emit gamma rays with trillion-electron Volt energies. The discovery was made possible by combining high-resolution radio and gamma-ray observations using three arrays of telescopes.
The Fermi telescope captured a hypnotic froth of gamma rays, revealing active galaxies called blazars flare up and fade out. The movie shows the entire sky as northern and southern halves, with bright colors indicating greater numbers of detected gamma rays.
A recent gamma-ray burst observed by the Fermi Gamma-ray Space Telescope is the most extreme recorded to date, with energies exceeding those of 9,000 ordinary supernovae. The blast's tremendous power and speed make it a significant finding in the field of gamma-ray bursts.
Astrophysicist Neil Gehrels receives the Henry Draper Medal for his groundbreaking work on gamma-ray bursts and active galactic nuclei. His leadership of NASA's Swift Mission has significantly advanced astronomers' understanding of these phenomena.
Fermi Gamma-ray Space Telescope has discovered 12 new gamma-ray-only pulsars and detected pulses from 18 others. The finds are challenging our previous understanding of how pulsars work, with gamma rays now believed to originate far above the neutron star.
Scientists have discovered a 10,000-year-old stellar corpse that only pulses in gamma rays, providing fundamental insights into the behavior of collapsed stars. The pulsar, located about 4,600 light-years away, emits 1,000 times the energy of our sun and is thought to be part of a larger population of similar objects.
Astronomers have discovered a pulsar that blinks only in gamma-rays, providing new insights into stellar evolution. The pulsar, located in the CTA 1 supernova remnant, is thought to be part of a large population of similar objects, offering researchers a unique way to study stars in our universe.
The Gamma-Ray Large Area Space Telescope (GLAST) will study the gamma-ray sky in unprecedented detail, revealing extreme astrophysical processes like pulsars and supermassive black holes. The mission aims to comprehend the origin and distribution of dark matter.
The Suzaku X-ray observatory has provided new insights into cosmic powerhouses, identifying pulsar wind nebulae as the source of high-energy gamma rays. The observations also suggest that these objects are accelerating mostly protons, leading to a better understanding of the origin of cosmic rays.
The Gamma-ray Large Area Space Telescope (GLAST) spacecraft has successfully completed two environmental tests and is now undergoing thermal and vacuum testing at the Naval Research Laboratory. The satellite will study extreme universe phenomena, including black holes and gamma-ray bursts.
The $20 million VERITAS telescope system, developed by Iowa State researchers, is the northern hemisphere's most sensitive instrument for detecting gamma rays. With improved data resolution, scientists can ask more precise questions about space objects and phenomena, such as supermassive black holes and dark matter.
Astrophysicists discovered a mechanism that produces high-energy gamma rays from the Milky Way's black hole, accelerating protons to unprecedented speeds. The process creates high-energy gamma rays through collisions between accelerated protons and hydrogen gas.
The H.E.S.S. collaboration has discovered gamma-ray emission from a complex of gas clouds near the Milky Way Galaxy's centre, revealing a prehistoric particle accelerator. The density of cosmic rays exceeds that in the solar neighbourhood, suggesting recent acceleration.
Researchers have detected gamma rays from radioactive aluminium (26Al) originating from the central regions of the Galaxy, indicating an ongoing process of new atomic nucleus production. The estimated total amount of radioactive 26Al is equivalent to three solar masses, corresponding to a galactic rate of supernovae every 50 years.
Scientists detected gamma rays in thunderstorms, contradicting a long-held theory. The study found lightning strokes preceding the gamma rays, suggesting a negative cause-and-effect relationship.
A massive gamma-ray flare from a magnetar was detected by the RHESSI satellite, emitting as much energy in two-tenths of a second as the sun gives off in 250,000 years. The event's immense power suggests a solution to the origins of short-duration gamma ray bursts.
Astronomers study remnant of 1,000-year-old supernova to solve long-standing puzzle of cosmic ray origin. They create gamma-ray image using Cherenkov radiation, providing first unequivocal proof that supernovae produce galactic cosmic rays.
Astronomers have detected high-energy gamma rays emanating from the center of the Milky Way galaxy, sparking debate about the nature of these mysterious emissions. The observation suggests a giant supernova explosion as the possible source, which could accelerate cosmic gamma rays to unprecedented energies.
Researchers at the University of Durham are using the H.E.S.S. telescope array to investigate extreme cosmic environments and detect gamma-ray sources, including supernova remnants and active galactic nuclei. The project seeks to shed light on the origin of cosmic rays, which bombard Earth from space.
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.
A new study suggests that most gamma radiation reaching Earth is leftover energy from massive shock waves caused by gravitational forces. The collision of electrons with low-energy photons could be a sign of ordinary matter captured within intergalactic clouds, shedding light on the 'missing matter' puzzle.
The Cangaroo II telescope detects gamma rays emitted by black holes and their surrounding electric and magnetic fields. Researchers aim to study the enormous effect of black holes on galaxy energy and evolution.
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
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.
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.
A new gamma-ray telescope will reveal new views of binary stars, black holes, and pulsars, shedding light on violent stellar explosions. The instrument, built by Columbia physicist Elena Aprile, will measure gamma rays between 300,000 to 30 million electron-volts, helping scientists understand element creation.
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.
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.