A team of astronomers has discovered a superluminous supernova in a spiral galaxy, which is rich in elements heavier than hydrogen and helium. This discovery challenges current ideas about the origin of such powerful explosions.
Researchers at Northwestern University discovered that up to half of the Milky Way's matter may have originated from distant galaxies through intergalactic transfer. This phenomenon, identified in simulations, shows that gas flows from smaller galaxies to larger ones, such as the Milky Way, forming stars.
A team of astronomers discovered a rare superluminous supernova in a distant galaxy 10 billion years ago. The brilliant explosion, one of the brightest ever recorded, occurred at cosmic high noon when the rate of star formation was at its peak.
Astronomers detected a rare superluminous supernova, one of the brightest ever seen, in a distant galaxy 10 billion light years away. The explosion occurred during the cosmic high noon period, when star formation peaked 3.5 billion years after the Big Bang.
Researchers generate high-energy shock waves in a laboratory setting, simulating the formation of supersonic shock waves that propel cosmic rays and particles. This breakthrough enables new studies on the acceleration of astrophysical particles and complements present remote sensing observations.
Researchers use ALMA to capture intricate 3-D rendering of newly formed molecules inside the supernova remnant, revealing previously undetected molecules such as formyl cation and sulfur monoxide. The study provides new insights into the physical instabilities inside a supernova and its impact on the surrounding interstellar space.
Scientists at Cardiff University have discovered new molecules, including formylium and sulphur monoxide, within the remnants of Supernova 1987A. This suggests that supernovae can create clouds of molecules and dust at extremely cold temperatures, similar to those in stellar nurseries where stars are born.
Scientists at the University of Oxford are recreating supernovae in a laboratory using lasers, allowing them to study the properties of these explosive events. This research is helping scientists better understand the origins of our universe and the formation of elements heavier than hydrogen and helium.
Astronomers Dr Jane Greaves and Dr Wayne Holland propose a new model for forming planets in the aftermath of a supernova explosion. They suggest that material caught up in the bow-wave around a moving neutron star could provide raw materials for future planet formation. Further data from ALMA is needed to confirm this theory.
Researchers find strong support for neutrino-driven supernova explosions, where neutrinos power the blast. The study confirms the theory using computer simulations and observations of radioactive elements in Cassiopeia A.
Researchers found a dying star that fizzled out and left behind a black hole, shedding light on why massive stars rarely explode as supernovae. The discovery could help explain the origins of supermassive black holes.
Astronomers discovered a massive star that collapsed into a black hole without exploding as a supernova, challenging the typical view of star formation. The study suggests that up to 30% of massive stars may quietly collapse into black holes without producing a supernova.
Astronomers using the VLA discovered a bright new object near Cygnus A's core, suggesting it could be either a rare supernova explosion or an outburst from a second supermassive black hole. The object's characteristics indicate it may have formed when the galaxy merged with another.
Astronomers have produced a highly-detailed image of the Crab Nebula by combining data from telescopes spanning nearly the entire electromagnetic spectrum. The image reveals intricate details about the nebula's structure and interactions with fast-moving particles and magnetic fields.
The Crab Nebula has been extensively studied, yet astronomers still have much to learn. By combining data from multiple telescopes, a team of scientists gained new insights into the object's complex physics.
Astronomers report the discovery of a binary solar-type star inside the supernova remnant RCW 86, with calcium abundance exceeding the solar one by a factor of six. This finding suggests that the supernova might belong to the rare type of calcium-rich supernovae.
Astronomers have discovered a unique star in the constellation of Lacerta, which is millions of times closer to Earth than the galaxy NGC 7250, allowing it to overpower its light
A large, wispy shell of gas, Sh2-308, is blown out by intense radiation from the extreme Wolf-Rayet star EZ Canis Majoris. The star's ongoing activity pushes the bubble to grow bigger and farther apart.
A team of international astronomers has discovered a magnified Type Ia supernova, allowing for precise measurements of the universe's expansion rate and dark energy. The discovery uses gravitational lensing to amplify the light from a
Astronomers have captured images of a Type Ia supernova appearing in four different locations on the sky due to gravitational lensing. This rare event has opened up new possibilities for measuring the rate of the Universe's expansion with unprecedented accuracy and understanding the distribution of matter.
Astronomers detected four images of the same supernova, a rare find, due to precise alignment with a foreground galaxy. This extreme case of gravitational lensing offers opportunities to study Type Ia supernovae and their role in cosmology.
A team of astronomers used the Hubble Space Telescope to analyze four images of a gravitationally lensed Type Ia supernova, measuring the expansion of the Universe without theoretical assumptions. The discovery provides clues about the Universe's expansion rate and has implications for cosmology.
An international team of physicists and astronomers has detected for the first time multiple images from a gravitationally lensed Type Ia supernova. The observations suggest that this phenomenon can be used to test key cosmological theories about the accelerating expansion of the universe and the distribution of dark matter. By analyzi...
Researchers discovered that massive stars can exhibit instability for several months before a supernova explosion, creating a dense gas shell around themselves. This insight came from analyzing data collected by the Palomar Transient Factory telescope network.
Astronomers identify sun-like star associated with a Type Ia supernova, sparking investigation into its potential role in the white dwarf's demise. Further studies are needed to confirm if this star is indeed the culprit behind a white dwarf's fiery explosion.
Astronomers have discovered the youngest and most distant galaxy ever seen, containing an abundance of interstellar dust formed by earlier star deaths. This discovery provides new information on when the first supernovae exploded and sheds light on the early Universe.
The supernova has continued to fascinate astronomers with its spectacular light show, located in the nearby Large Magellanic Cloud. Recent studies using NASA's Hubble Space Telescope and Chandra X-ray Observatory have provided unique insight into the early stages of gas dispersal after a star's death.
New research suggests that pure iron grains are extremely rare in the universe, contrary to previously thought, and may be forming invisible metal particles. A study published in Science Advances used a rocket-based experiment to simulate the formation of pure iron grains in space, revealing grain formation is highly unlikely.
Astronomers detected a compact molecular cloud with unusual motion near the supernova remnant W44, suggesting the presence of a hidden black hole. The black hole is estimated to be between 3.5 and 36 times more massive than the sun, sparking debate over its origin.
The study provides new insights into the distinctive geometry of pulsars and their emission signatures. The researchers found that the orientation of pulsars' spin and magnetic axes significantly affects what emissions are seen on Earth.
Researchers at University of Chicago and Wayne State University reaffirm the reliability of Type Ia supernovae for measuring cosmic distances. The findings contradict recent claims that these supernovae are inconsistent in their brightness.
Astronomers discovered a rare event where a star was destroyed by a massive black hole's gravitational tides, producing an unusually bright flash of light. The event occurred in a distant 'red' galaxy with older stars, defying typical supernova models.
A team of astronomers discovered that a massive flare in a distant galaxy was actually a tidal disruption event caused by a rapidly spinning supermassive black hole. The finding marks the first time a TDE has been used to study black hole spin, providing new insights into stellar death.
A spinning supermassive black hole destroyed a Sun-like star, causing the most luminous supernova ever recorded. The observation is attributed to a tidal disruption event rather than an extraordinary bright supernova.
A new study published in Nature Communications presents evidence suggesting that a low-mass supernova played a crucial role in the formation of our solar system. The research team analyzed short-lived radioactive nuclei found in meteorites and discovered unique 'fingerprints' that point to a low-mass supernova as the trigger.
Astronomers detected carbon monoxide gas indicating large quantity of molecular hydrogen, suggesting formation of a single, gigantic galaxy. The cloud of cold gas is estimated to be three times the size of the Milky Way Galaxy.
A team led by Professor Yong-Zhong Qian uses new models and meteorite evidence to show a low-mass supernova triggered the formation of our solar system. The study found that short-lived nuclei in meteorites are consistent with a low-mass supernova trigger, supporting the theory that this event played a key role in solar system formation.
The Super-Kamiokande detector is equipped with a new computer system to monitor neutrinos from nearby supernovae in real-time. This allows scientists to assess the significance of signals within minutes and issue early warnings to research centers worldwide.
Dense molecular gas disks are supplying gas directly to supermassive black holes at galaxy centers. The growth of supermassive black holes is enhanced by strong turbulence generated by supernova explosions in these disks.
Research found that circumbinary planets can survive the late stages of their binary star's life by moving to wider orbits. Many such planets are likely to escape destruction and potentially become habitable for a short period.
Astrophysicists propose that inspiraling white dwarfs could produce a type of explosion that matches Type Ia supernovae. The model suggests that resonance in the binary orbit of the stars causes rapid jumps in energy that can lead to detonation.
Researchers at the University of Surrey have discovered hundreds of undetectable black holes within a globular cluster, overturning old theories on their formation. The study uses advanced simulations to map the cluster and its behavior, revealing the effects of these massive objects on the surrounding stars.
Researchers find evidence of two separate eruptions in the mid-13th and mid-16th centuries, and another in the 19th century, revealing a more violent history for the star system. The team uses NASA's Hubble Space Telescope images to track the movement of gas ejected by Eta Carinae.
Researchers found a time-resolved supernova signal in biogenically produced crystals from Pacific Ocean sediment cores, indicating the solar system spent 1 million years transiting through a supernova's debris. The signal was first detectable at 2.7 million years ago and ended around 1.7 million years ago.
Astronomers have peer into a nearby star's past, using low-frequency radio observations to fine-tune our understanding of stellar explosions. The team found the red supergiant lost matter at a slower rate and generated slower winds, improving knowledge of space composition.
Researchers used the Gran Telescopio CANARIAS to observe a superluminous supernova almost from its occurrence, revealing surprising behavior including an initial increase in brightness followed by a decline and later stronger increase. The study sheds new light on these rare events, which are up to 100 times more energetic than Type 1a's.
Researchers have found a unique triple-bubble structure in the interstellar medium of galaxy M33, consisting of three concentric supernova shells. This discovery provides insights into the complex feedback processes that govern star formation and the dissemination of metals produced in massive stars.
A new study reveals that neutrinos produced in the core of a supernova are highly localized compared to all other known sources. Theoretical wave packet size is irrelevant in simpler cases, providing a more solid foundation for standard neutrino behavior theories.
The Crab Nebula is home to a spinning neutron star with a 'heartbeat' radiation signature, emitting clock-like pulses of energy. The neutron star is surrounded by expanding debris and glowing gas, revealing the intricate details of this cosmic object.
Researchers analyzed UV spectrum of BD+44 493, a second-generation star thought to have been enriched by one of the first stars. They found phosphorus, sulfur, and zinc, which reveal the star was likely massive and exploded as a supernova.
Astronomers using OISTER telescope consortium in Japan have discovered the origin of 'extraordinary supernovae', which are brighter than normal ones. The 'accretion' scenario supports the discovery, where material ejected from a white dwarf is responsible for the emission.
A giant star exploded 30 million years ago in a galaxy near Earth, releasing energy equivalent to 100 million suns. The analysis revealed the star's mass, radius, and chemical composition before its spectacular demise.
A rare type of iron nucleus, with a half-life of 2.6 million years, serves as a 'clock' to measure the distance between Earth and the source of galactic cosmic rays. The data suggest that nearby supernovae in massive star clusters are responsible for creating these nuclei.
Scientists have discovered a nearby supernova's ash continuing to fall on Earth, with rare iron-60 isotope detected in cosmic rays. The findings suggest another supernova occurred near the previous one, contributing to the ongoing acceleration of these nuclei.
Researchers at TUM and USA colleagues have discovered unusually high concentrations of radioactive 60Fe in lunar samples from Apollo missions 12, 15 and 16. This evidence supports a supernova hypothesis, suggesting that one or more explosive events occurred close to our solar system approximately two million years ago.
An international team found radioactive iron-60 in sediment and crust samples from the Pacific, Atlantic, and Indian Oceans, indicating a series of massive supernovae near our solar system. The debris is dated to 3.2-1.7 million years ago and coincides with Earth's cooling period.
Scientists are using computer models to simulate the production of heavy elements in supernovae and neutron-star mergers. The study aims to identify areas where future experiments can reduce uncertainties in nuclear models.
Scientists found that magnetars could boost the energy source of super-luminous supernovae, which are 10-100 times brighter than normal supernovae. Calculations suggest that rapidly spinning magnetars could power these extreme events.
Astronomers capture shock breakout of a supernova for the first time in visible light, revealing unexpected diversity in cataclysmic stellar events. The observations, made using NASA's Kepler space telescope, matched up well with mathematical models of Type II explosions.
Recent measurements from the LOFAR radio telescope have provided new insights into the properties of cosmic rays, including a surprisingly high number of light particles at high energies. The KIT simulation code CoREAS has enabled precise analysis and interpretation of these signals.