Articles tagged with Supernova Remnants
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A team of researchers at Kyoto University used X-ray spectroscopy to measure the amount of chlorine and potassium inside a supernova remnant, revealing that these elements were created in intense environments deep inside stars. The study suggests that strong mixing inside massive stars can enhance the production of these elements.
A new type of supernova has been discovered, offering a rare glimpse into the depths of massive stars. The star, dubbed SN2021yfj, had lost its outer layers while still 'alive,' revealing a previously unknown inner layered structure and exposing hidden sites where heavy chemical elements are formed.
Researchers have found visual evidence of a double detonation process in the remains of a star that exploded twice, providing new insights into the mechanism behind Type Ia supernovae. This discovery confirms a long-standing hypothesis and offers a tangible explanation for these cosmic events.
A new study suggests that violent supernovae caused at least two mass extinction events in Earth's history, including the late Devonian and Ordovician extinctions. Researchers believe a nearby supernova could have stripped the planet's atmosphere of ozone, sparking acid rain and exposing life to harmful ultraviolet radiation.
Researchers have observed a rare metal-poor supernova, providing valuable information about the early universe. The study revealed that this supernova was distinct from others in nearby galaxies, with unique properties such as a steady brightness period and rapid spin.
A recent study reveals that fast radio bursts are more commonly associated with massive and metal-rich star-forming galaxies. This suggests that magnetars, the thought-to-be-triggers of FRBs, likely form in environments conducive to stellar mergers. The discovery was made using Caltech's Deep Synoptic Array-110 project.
Researchers from DTU have discovered a neutron star that rotates at an astonishing 716 times per second, making it one of the fastest-spinning objects ever observed. The neutron star is part of an X-ray binary star system and is located in the Sagittarius constellation.
Astronomers have studied the last unexplained historical supernova from 1181 AD, known as SN 1181, in detail. The team discovered a 'zombie star' at its center and dandelion-shaped filaments emanating from it.
The James Webb Space Telescope has revealed intricate patterns of shells, holes, and filaments in the supernova remnant Cassiopeia A, providing insights into molecular formation and destruction processes. CO molecules are critical indicators of cooling and chemical processes that lead to dust condensation.
Researchers recreated the structure of supernova remnant SN 1181 using a new computer model, explaining its double shock formation. The study also found that high-speed stellar winds may have started blowing from its surface within the past 20-30 years.
The team gathered data that helps clarify the Crab Nebula's history, suggesting a weak iron core-collapse supernova as an alternative to electron-capture explosions. The study also mapped dust distribution within the nebula for the first time, revealing warmer dust in outer filaments and cooler grains near the center.
Astronomers have detected a neutron star spinning at an unprecedentedly slow rate, defying the typical mind-bending speeds of these ultra-dense stars. The object emits radio signals every 54 minutes, offering new insights into its complex life cycle and potential implications for our understanding of stellar objects.
Astronomers uncover evidence of a massive star's quiet demise into a black hole without a supernova explosion. The VFTS 243 system shows minimal signs of an explosion, offering insight into stellar evolution and collapse theories.
The brightest gamma-ray burst (GRB) ever recorded was caused by the collapse of a massive star, according to Northwestern University researchers. Despite extensive searches, no evidence of heavy elements like platinum and gold was found.
The James Webb Space Telescope has found direct evidence for emission from a probable young neutron star at the site of the recently observed supernova SN 1987A. Spectral analysis revealed strong signals due to ionized argon and five times ionized argon, indicating high-energy radiation from the compact object.
A new study published in Science provides conclusive evidence for the presence of a neutron star at the center of supernova SN 1987A, solving a decades-long mystery. The detection was made using the James Webb Space Telescope and reveals narrow emission lines from ionized argon and sulphur atoms.
Researchers use James Webb Space Telescope to observe Supernova 1987A and detect ionised argon and sulphur atoms, providing conclusive evidence for a neutron star's presence. The discovery sheds light on the formation of heavy elements and the nature of compact objects in supernovae.
Researchers utilize the SETI Ellipsoid method to identify potential technosignatures in continuous sky surveys, enhancing detection capabilities. The method compensates for uncertainties in signal arrival times using observations spanning up to a year.
Researchers found a direct connection between massive star deaths and compact remnant formation, using observations of a nearby galaxy's SN2022jli supernova. The team detected periodic movements and energy signatures indicating a neutron star or black hole sucking up matter from its companion star.
Researchers found a correlation between light precision metals like silver and rare earth nuclei like europium, indicating a consistent process operating during heavy element formation. The pattern provides a clear signature of fission creating these elements.
Astronomers confirm that a stellar corpse is the source of repeated energetic flares observed after a distant star's explosive death. The team detected at least 14 irregular light pulses over a 120-day period, likely driven by processes such as rapid rotation or strong magnetic fields.
A new study using CALET data finds evidence for nearby, young sources of cosmic ray electrons, contributing to a greater understanding of the galaxy. The study suggests that these high-energy electrons originate in supernova remnants, offering insights into the galaxy and its sources.
Researchers from Helmholtz-Zentrum Dresden-Rossendorf are studying near-Earth cosmic explosions to understand their potential impact on the Earth's biosphere. They found that ejected debris can reach our solar system, with some isotopes, such as iron-60 and plutonium-244, potentially coming from supernovae or other galactic events.
Researchers utilized the IXPE telescope to capture the first polarized X-ray imagery of SN 1006, revealing a connection between magnetic fields and high-energy particle outflow. The discovery expands scientists' understanding of supernovae remnants.
A WVU astronomer is searching the Milky Way for debris left behind by supernovas, with $331,170 in NSF funding. He hopes to discover new supernova remnants using radio wavelength data from telescopes and machine-learning software.
Researchers discovered a new type of astronomical object - a massive magnetic helium star that may evolve into a magnetar. The star has a phenomenally powerful magnetic field, about 43,000 gauss, and will eventually collapse into a neutron star with an even stronger magnetic field.
Researchers at Ohio State University have developed a new framework for studying neutrino self-interactions using supernovae. They found that in the burst case, unprecedented sensitivity to neutrino self-interactions is possible even with sparse data from SN 1987A and conservative analysis assumptions.
Researchers have found evidence of a demolition-derby-like collision of stars or stellar remnants in the chaotic region near an ancient galaxy's supermassive black hole. This suggests that stars can meet their demise in some of the densest regions of the Universe, potentially creating gamma-ray bursts.
The Dark Energy Camera has captured a rare and detailed view of the supernova remnant from 185. This event is significant as it marks the first-ever documented supernova. The team aims to better understand dark energy's impact on astronomical observations.
A new study published in Science found that a highly magnetised dead star, known as a magnetar, is likely to have a solid surface with no atmosphere. The research team used data from the NASA satellite IXPE to observe the polarisation of X-ray light emitted by the star, which revealed a signature consistent with a solid crust.
A new study has created the first map of the Milky Way's ancient dead stars, which reveals a 'galactic underworld' stretching three times the height of the galaxy. The map shows that almost a third of objects have been flung out from the galaxy, with neutron stars and black holes formed when massive stars collapse.
Astronomers have long sought the launch sites for high-energy protons in our galaxy, and NASA's Fermi Gamma-ray Space Telescope has confirmed that a supernova remnant is just such a place. The shock waves of exploded stars boost particles to speeds comparable to light, producing a tell-tale glow in gamma rays.
Scientists have found evidence for a young and extremely powerful neutron star, dubbed VT 1137-0337, in a dwarf galaxy 395 million light-years from Earth. The pulsar is thought to be as young as 14 years old and has the strongest magnetic field of any known object.
A new study suggests that the Hypatia Stone, discovered in Egypt, may be the first tangible evidence on Earth of a supernova type Ia explosion. The stone's unique chemistry and elemental composition contradict conventional views of solar system formation, potentially revealing a long-hidden secret about our cosmic neighborhood.
Researchers used computer modeling to simulate the long-term evolution of a hypothesized type of supernova, known as D6. The study found that remnants of type Ia explosions are not necessarily symmetric, offering new insights into supernova physics. This finding has significant implications for using Ia supernovae as cosmic yardsticks.
The Imaging X-ray Polarimetry Explorer (IXPE) mission enables new measurements of cosmic X-ray sources, such as pulsars, black holes, and neutron stars. With its state-of-the-art telescopes and detectors, IXPE will provide high-quality polarization data of various sources, including supernova remnants, active galaxies, and blazars.
Researchers have captured a 1,000-year-old supernova in 3D images, revealing unprecedented details about the elements ejected during a star's explosion. The study provides a three-dimensional map of these elements, shedding light on the conditions at the time of the explosion and the importance of asymmetries in supernovae.
Researchers have solved the 900-year-old mystery of the Chinese supernova of 1181AD by identifying a matching nebula and star in the Milky Way. The Pa30 nebula, surrounding Parker's Star, matches the profile, location, and age of the historic supernova.
Physicist Eve Armstrong aims to understand the origins of elements heavier than iron using weather prediction technique data assimilation. With a two-year NSF EAGER grant, she and her team will predict whether supernova stardust gave rise to these heavy elements.
Astronomers have discovered a unique 'heart-shape' with intricate gas filaments at the centre of the Crab Nebula. The new 3D reconstruction challenges traditional supernova theories and provides unprecedented insights into the explosion.
Researchers used Hubble's imagery to wind back the clock on a supernova remnant, pinpointing its age and centre. The study found that light from the blast arrived at Earth 1700 years ago, during the decline of the Roman Empire.
Scientists detected high levels of the radioactive isotope 60Fe in deep-sea sediment samples, indicating exposure to supernova ejecta. The findings suggest that supernova-produced 60Fe permeates the interstellar medium and has been deposited on Earth over the past 33,000 years.
A lab machine has been developed to mimic the explosion of a giant star, allowing researchers to study the formation of supernovas and their impact on galaxy evolution. The device replicates the blast wave's effects on gas layers, enabling scientists to better understand the creation of beautiful swirls in supernova remnants.
Scientists created a scaled-down shock wave in the lab, mimicking supernova remnants. The study found that turbulent electromagnetic fields within the shock boost electron speeds, allowing particles to escape and gain even more speed.
A radio telescope in the Western Australian outback has captured a new view of the Milky Way's centre, revealing remnants of 27 massive stars that exploded as supernovae. The data comes from the GaLactic and Extragalactic All-sky MWA survey, which used low-frequency radio waves to map the sky.
Astronomers have found a pulsar that has escaped the debris of a supernova explosion and is now speeding away at nearly 700 miles per second. The discovery provides important insights into how pulsars can gain speed from supernovae.
Astronomers have directly observed the magnetism in Supernova 1987A, a dying star that appeared thirty years ago. The detection reveals a degree of order in the magnetic field, contrary to chaotic expectations.
Astronomers have discovered an isolated neutron star with low magnetic field located beyond our Milky Way galaxy using the MUSE instrument on ESO's Very Large Telescope in Chile. The neutron star is surrounded by a ring of gas that includes neon and oxygen.
The Water Recovery X-ray rocket, WRX, will test a newly-developed X-ray spectrograph and study the X-rays from a supernova remnant in the Milky Way galaxy. The mission will provide information about the conditions in the Vela supernova remnant, including temperature, density, chemical composition, and ionization state.
Astronomers have discovered a white dwarf with low mass, high velocity and strange composition that may be the remnants of a Type Iax supernova. The calculated age of the explosion suggests it occurred between five and 50 million years ago.
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.
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.
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.
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.
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.
NuSTAR's observations confirm a highly asymmetric Supernova 1987A explosion, with X-ray emissions revealing explosive speeds of heavy elements. This study validates scientific assumptions about core collapse supernovae and challenges symmetrical explosion models.
Researchers made direct observations of cosmic dust resulting from an ancient supernova at the Milky Way's center, supporting the theory that supernovae produce dust in galaxies of the early universe. The study provides new insights into the origins of dust, a crucial component in star and planet formation.
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.
The High Energy Stereoscopic System (H.E.S.S.) has detected three powerful gamma-ray sources in the Large Magellanic Cloud, including a pulsar wind nebula and a supernova remnant. These discoveries provide new insights into the formation of cosmic structures and the evolution of galaxies.
Researchers have used radio telescopes in Australia and Chile to observe the remnant of Supernova 1987A, providing insights into the explosion's aftermath. The team has also developed a three-dimensional simulation that reproduces observed features, including the persistent one-sidedness in radio images.