Articles tagged with Stellar Explosions
A team from the Instituto de Astrofísica de Canarias has found a new method to measure star formation rates in galaxies using radio emission. The study reveals that radio waves are an ideal tracer for estimating star formation rates, unaffected by interstellar dust and not requiring combination with other tracers.
Researchers have discovered that cosmic heavy metals, such as gold and platinum, can be used to trace the history of galaxies. The study, published in Nature, suggests that the collision of dense stars in the universe can forge these heavy elements and provide insights into galaxy formation.
Researchers use ALMA to accurately measure the mass of a supermassive black hole at the center of galaxy NGC 1332, shedding light on how galaxies and their black holes form. The findings suggest a coordinated growth between galaxies and their central black holes.
Astronomers have identified a type of gas found in galaxy voids that appears to fuel star formation under certain conditions. Researchers used radio telescopes to measure atomic gas levels in galaxies with gamma-ray bursts, finding large amounts of the gas near these events.
Harvard-Smithsonian astronomers created a new 3-D map of the interior of Cas A using a CAT scan equivalent. They found six massive cavities, or bubbles, that likely formed from radioactive nickel generated during the supernova explosion.
Researchers recreated isotopes formed when stars explode, shedding light on heavy element creation essential for life. This study helps map the pathway for creating life-supporting elements in the universe.
Astronomers find compact, young galaxies shut down their prodigious star production due to a lack of cool dense gas, rather than supermassive black holes. The energy from the star formation itself creates a shortage of gas within the galaxy.
The NASA Swift satellite detected a series of powerful stellar flares from the nearby red dwarf star DG CVn, with temperatures reaching 360 million degrees Fahrenheit. The flares were triggered by rapid spin and amplifying magnetic fields, making them one of the longest-lasting events ever recorded.
Astronomers have discovered a compact galactic core, nicknamed Sparky, which is seen as it appeared 11 billion years ago. The infant galaxy contains twice as much mass as the Milky Way and is producing 300 stars per year, a rate three times faster than our galaxy.
Astronomers have observed the earliest stages of massive galaxy construction, dubbed 'Sparky', which contains about twice as many stars as our Milky Way. The discovery was made possible through combined observations from NASA's Hubble and Spitzer space telescopes.
A historic epidemic of sea star wasting syndrome has exploded along Oregon's coast, with 30-50% of ochre sea stars affected and potentially leading to local extinctions. The outbreak could disrupt the marine intertidal ecosystem, causing widespread damage.
Researchers have detected circularly polarized light from a recently formed black hole, confirming a theoretical model. The discovery was made using the VLT telescope and is considered an extraordinary event due to its high degree of polarization.
Scientists discovered that massive galaxies in the early universe were formed by explosive star formation triggered by galaxy collisions. This theory contradicts the traditional view that galaxies grew larger over time through constant star formation and mergers.
A team of astronomers from Cardiff University has discovered a noble gas molecule, argon hydride, in the Crab Nebula. The find provides new insights into the chemistry of outer space and challenges previous assumptions about the conditions necessary for such molecules to form.
Theoretical calculations reveal previously unknown layers where nuclear reactions within the crust cause rapid neutrino cooling, altering our understanding of neutron star hot surfaces. Researchers now face new questions about the star's thermal dynamics and discovery potential of the Facility for Rare Isotope Beams.
Gamma-ray burst GRB 130427A was observed by NASA satellites and ground-based telescopes, revealing a spike in high-energy gamma-rays that defies expectations. The event challenged current theoretical understanding of internal and external shock waves producing these bursts.
Astronomers have observed a neutron star system known as Circinus X-1, where one of the companion stars is a compact neutron star. The system flared twice during observation, with KAT-7 capturing detailed radio images of the event.
Astronomers have detected giant outflows of charged particles from the center of our galaxy, stretching across half the sky and emitting an enormous amount of energy. The outflows were found to be driven by star formation and are carrying strong magnetic fields that may play a key role in generating the galaxy's overall magnetic field.
Researchers at Tel Aviv University develop method to observe stars that formed when the universe was 180 million years old. By detecting radio waves from hydrogen atoms, they reveal patterns in the sky indicating early galaxies, providing insight into the universe's origins.
Astronomers have observed a unique neutron star system, T5X2, exhibiting marginally stable nuclear fusion at high accretion rates. The RXTE data resolves a long-standing gap between theoretical predictions and observational evidence, shedding light on the complex processes governing thermonuclear explosions.
A neutron star spiraling into its companion star caused a unique gamma-ray burst with varying wavelengths and characteristic radii. The Helium Merger Model, developed in 1998, explained the unusual properties of the burst, which may be part of a new class of bursts.
Astrophysicists with VERITAS detect pulsed gamma rays above one hundred thousand million electron volts, defying current pulsar models. The finding is causing researchers to consider new theories about gamma-ray production.
Astronomers confirm 13.14 billion light-year distance for GRB 090429B, making it contender for most distant object detected, and shedding light on the cosmos' earliest stars and galaxies.
A gamma-ray burst, GRB 090429B, has been identified as a potential candidate for the most distant object in the universe at an estimated distance of 13.14 billion light years. The burst was detected by NASA's Swift satellite and is believed to be extremely likely, with a 99.3% chance, to be the most distant cosmic explosion.
Detecting raging storms of molecular gas streaming away from galaxies for the first time, Herschel reveals powerful outflows that could halve a galaxy's star-forming capacity within one million years. This discovery offers insights into galactic evolution and negative feedback mechanisms.
Researchers found NGC 1266, an early-type galaxy, expelling molecular gas at high speeds, potentially leading to its transformation into a 'red and dead' state. The galaxy's gas loss could be a key mechanism in the evolution of galaxies from star-forming spirals to gas-poor red and dead galaxies.
Distant galaxies in the early Universe are creating 1,000 new stars per year, exceeding our galaxy's star formation rate. These galaxies contain enormous amounts of raw material for new stars, suggesting a higher gas content than previously thought.
A team of researchers has made the first detailed observations of 'halo' gas clouds in our Galaxy, finding they contain hydrogen gas 700 times the mass of the Sun. These clouds are linked to earlier star formation and can fall back into the main body of the Galaxy, recycling material.
Most 'dark' gamma-ray bursts are found to be similar to normal bursts with an afterglow, but with nearly all visible light obscured by patchy dust. This suggests that gamma-ray bursts may help track star formation and death in distant galaxies.
A team of astronomers has discovered the most distant object in the universe, a gamma-ray burst located approximately 13 billion light-years away. This explosive event, dubbed GRB 090423, occurred when the universe was just 630 million years old and is providing valuable insights into the early universe.
Astronomers have discovered a gamma-ray burst from a star that died 630 million years ago, marking the most distant cosmic explosion ever seen. The burst, dubbed GRB 090423, is approximately 13 billion light-years away.
A new study published in Science resolves the mystery of how massive stars can form without blowing away the gas and dust that feed their growth. The research found that instabilities develop in the collapsing gas cloud, creating channels where radiation blows out into space while gas continues to fall inward.
Swift's Ultraviolet/Optical Telescope (UVOT) observes the chemical composition of comet atmospheres, while its X-Ray Telescope (XRT) studies gas and solar wind interactions. This research offers clues about comets' origins and the solar system.
Astronomers have observed the most detailed picture of a gamma-ray burst, detected by NASA's Swift satellite on March 19. The burst was so bright it became visible to human eyes and provided insights into the universe's most luminous explosions.
The brightest gamma-ray burst, GRB 080319B, provided a wealth of information on how stars explode. The team discovered that the jet directed towards Earth contained an ultra-fast component just 0.4 degrees across.
A rare and intense stellar flare was detected by NASA's Swift satellite from the normally quiet red dwarf star EV Lacertae. The flare, which lasted for 8 hours, would have sterilized life-bearing planets' surfaces if they were nearby.
Astronomers predict hundreds of rogue black holes, each several thousand solar masses, could be roaming the Milky Way. The discovery challenges current understanding of black hole formation and detection.
A team of astronomers discovered a long-duration gamma-ray burst (GRB) in the middle of nowhere, thousands of light-years from the nearest galaxy. The GRB's afterglow was bright and fast-fading, but there was no dense gas or dust to absorb its light.
The University of Delaware is building 'IceTop,' a surface array of detectors for the IceCube project, which aims to detect high-energy particles from space. The telescope will provide new insights into cosmic events and reveal their inner workings.
Researchers have built a new model that suggests neutron star surfaces run hotter than previously thought, releasing 10 times more heat. This helps explain the observed frequency of superbursts on such stars' surfaces, but scientists still don't know why they occur annually.
The study of gamma-ray burst (GRB) 060729 reveals a wider energy release and potential magnetar powering some GRBs. The XRT detected the GRB's afterglow for over 125 days, defying expectations.
Researchers at the University of Chicago have made a groundbreaking discovery in air bubble behavior, revealing that they can tear apart instead of pinching off. This phenomenon has significant implications for our understanding of fluid dynamics and the equations that govern it.
Astronomers use Hubble Space Telescope to image two mysterious star types, including tiny, slow-burning stars and ancient, giant white dwarfs. The research pushes limits of observatory's capabilities, gathering data that will help refine theories about low-mass stars and the universe's age.
Researchers analyze gamma-ray burst GRB 050904 to understand the conditions of the early universe. The burst, detected in 2005, provides a probe to study the universe beyond the reach of large telescopes.
A team from MIT and Harvard found that a certain type of X-ray explosion common on neutron stars is never seen around their black hole cousins, indicating the presence of an event horizon. The absence of surface explosions called X-ray bursts suggests that gas released by nearby stars vanishes into a void.
Astronomers have found a massive star cluster in the Milky Way, consisting of 14 supergiants with a total mass of at least 20,000 solar masses. This discovery may challenge existing massive star formation models and provides valuable insights into the evolution of these stars.
A team led by Neil Gehrels' Swift science team detected the afterglow of a gamma-ray burst (GRB) with a redshift of 6.29, confirming Lamb and Reichart's earlier prediction from 1999. This discovery smashes the old distance record by 500 million light years.
X-ray flashes and gamma-ray bursts, two powerful cosmic explosions, have long been linked in theory. New satellite data, however, suggests that these events may not be as connected as previously thought, contradicting popular theories.
A recent study led by Professor Albert Zijlstra has found that up to 0.1% of a star's mass can be expelled during re-ignition, equivalent to 300 times the mass of Earth. This discovery suggests that part of the carbon in the universe may have come from these events, providing new insights into the formation of our planet.
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.
Astronomers have discovered a quadra-polar nebula with two disks formed at different times, challenging the companion-star-only model. The study, led by C. Robert O'Dell, used sharp new images from the Hubble Space Telescope to reconstruct the 3D structure of the Helix Nebula.
Astronomers from Johns Hopkins University confirm the Cygnus Loop is closer to Earth than previously thought, with a distance of 1,860 light years. The new findings were obtained using the Far Ultraviolet Spectroscopic Explorer (FUSE) satellite and provide an accurate starting point for understanding this important supernova remnant.
Researchers detected a sudden cooling of the star Rho Cassiopeiae in 2000, resulting in an unprecedented mass ejection into space. The star is now considered one of the brightest yellow hypergiants in the Milky Way, with a luminosity over half a million times that of the Sun.
Chandra has revealed unprecedented images of a blast wave from an exploding star, a flare from a brown dwarf, and a small galaxy being cannibalized by a larger one. The observatory's high resolution has enabled scientists to pinpoint sources of the X-ray background glow, leading to a better understanding of our universe.
Astronomers have discovered an expanding oxygen and neon ring in the remnants of a massive star explosion, providing unprecedented insights into the creation and dispersal of heavy elements. The findings suggest that these elements are necessary for life on Earth and could provide clues to the nature of supernovae.
A team of astronomers has used Chandra to map the distribution of silicon, sulfur, and iron in Cassiopeia A, a supernova remnant. The findings provide insights into how elements are produced in stars and their subsequent release into space.
Researchers found a direct correlation between the pattern of X-ray emission and the size of supernova remnants. Larger remnants exhibit brighter X-ray emission from their centers, suggesting changes in gas distribution as they age.
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.
Astronomers have discovered a large number of slow X-ray pulsars in supernova remnants, which are believed to be neutron stars with huge magnetic fields. These so-called magnetars rotate much slower than expected and are invisible to radio probes.
A team of scientists has discovered a young and previously unknown supernova remnant located just 700 light years away from the Vela supernova remnant. The remnant is exceptionally close to Earth, with an age of at most 1500 years, making it the nearest supernova remnant to have occurred during recent human history.