Astronomers are studying a mysterious gamma-ray emission from the center of the Milky Way galaxy, which is surprising given the presence of massive stars and black holes. The emission is thought to be caused by exotic particles such as dark matter or the decay of radioactive elements.
Researchers found evidence of cosmic dust forming around a dying star in a nearby galaxy, similar to those that formed soon after the Big Bang. This discovery provides insight into the early stages of the Universe and challenges the long-held theory that supernovae explosions are the primary source of dust.
The team's three-dimensional visualization provides clues about how supernovas form new stars and solar systems. The research also helped identify the chemical elements emerging from the exploded star, shedding light on the process of star formation.
A team of scientists has created a movie tracking the expansion and changes of Cassiopeia A over time, revealing slower-than-expected energy loss. The visualization also shows high-velocity plumes from the explosion, challenging current theoretical models.
A team of UBC researchers found that a mysterious force known as dark energy is responsible for the acceleration of the Universe, contradicting a theory that suggested the Earth was near the center of a giant void. The study used data from various sources, including the Wilkinson Microwave Anisotropy Probe satellite.
Researchers have captured a rare binary star explosion inside a planetary nebula, offering new insights into stellar evolution. The study predicts that the combined mass of the two stars could lead to a larger supernova explosion.
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.
Researchers at Carnegie Institution resolve solar system formation with detailed model of supernova triggering collapse. The 'Little Bang' theory suggests a supernova shock wave triggered the Sun and planets.
Scientists using Spitzer data have identified the precise event that produces the echo we see, revealing the supernova's first flash. The hot spots near the shattered remains of an exploded star are echoing the blast's first moments, powered by radiation from the supernova shock wave.
A team of astronomers has discovered a potential 'wild cousin' of the infamous exploding star supernova 1987A in a nearby galaxy. The newly found supernova, SN1996cr, exhibits similar characteristics to '87A and is an impressive 1,000 times brighter.
The survey uses baryon acoustic oscillations to measure the expansion of the universe. It will double the volume of space in which red luminous galaxies are studied, observing 10,000 square degrees of sky out to redshifts of z = 0.7.
Researchers propose that Eta Carinae's historic 1843 outburst was a fast blast wave similar to a supernova, but less energetic. This discovery challenges current theories and may indicate supermassive stars undergo periodic explosions before their final supernova.
The CLOUD experiment aims to understand the role of cosmic rays in cloud formation and climate change. By simulating cosmic ray intensity, researchers plan to uncover details of aerosol and cloud formation mechanisms.
Researchers are investigating SEP transport in 3D heliospheric magnetic fields to understand why some events occur without magnetic connection to the Sun. The goal is to assess cross-field diffusion's role in charged particle transport.
The IBM Blue Gene/P Intrepid supercomputer will have a new data analytics and visualization capability, complementing its distinction as the fastest computer in the world for open science. The system, nicknamed Eureka, will enable researchers to explore and visualize data produced by Intrepid.
Scientists have made direct measurements of the solar wind termination shock using Voyager 2 data, which could help understand how cosmic rays are produced. The observations reveal intense plasma wave turbulence and unexpected effects, sparking revisions to theories.
The study reveals that no more than 4% of energy loss is caused by gravitational waves, disproving a key hypothesis. The analysis provides valuable information about the pulsar and its structure, shedding light on the role of gravitational waves in its dynamics.
Researchers used LIGO data to analyze the Crab Pulsar, detecting signals that reveal no more than 4% of energy loss is due to gravitational radiation. The findings suggest other mechanisms, such as electromagnetic radiation and high-velocity particles, are responsible for the pulsar's slowing spin.
Astronomers have detected a giant ring around a rare and exotic star known as a magnetar, which was likely produced by a massive flare. The discovery provides valuable insights into the phenomenon associated with magnetars, a type of neutron star with incredibly strong magnetic fields.
A team of researchers, led by Stephanie Wachter and Vikram Dwarkadas, investigated the mysterious ring surrounding magnetar SGR 1900+14. They concluded that a powerful flare from the magnetar formed the ring, which measures seven light-years across.
Astronomers captured X-ray outburst from supernova SN 2008D, shedding light on early processes. The explosion was likely from a massive star with retained helium layer, providing valuable information for understanding stellar deaths.
Astronomers have witnessed a star dying in real-time for the first time, marking a major breakthrough in understanding supernovae. The team used NASA's orbiting Swift telescope to detect an extremely luminous X-ray blast from the explosion, confirming that it was indeed a supernova.
Astronomers have observed a rare 'normal' supernova for the first time at its moment of birth, thanks to NASA's Swift satellite. The discovery provides unique insights into how these massive star explosions occur, with the radiation pattern giving scientists the clearest picture ever.
Astronomers have caught a supernova explosion in the act, providing valuable insights into the process. The observation, made possible by NASA's Swift satellite, has helped scientists form a detailed picture of star explosions and shed light on long-standing puzzles.
Astronomers have tracked a recent supernova explosion in the Milky Way galaxy using NASA's Chandra X-ray Observatory and NRAO's VLA. The discovery confirms the supernova is about 140 years old, making it the youngest recorded in the galaxy.
Dr. Stephen Reynolds and his team discovered the youngest known supernova remnant G1.9+0.3, estimated to be around 100-140 years old, using Chandra X-Ray Observatory images from 2007 and 1985. The discovery suggests that a supernova explosion occurred relatively recently, providing insights into the life cycle of galaxies.
Scientists have discovered a timing mechanism in neutron stars that allows them to predict when incredibly powerful X-ray bursts will occur, releasing energy equivalent to 100 hydrogen bombs exploding simultaneously.
A team of astronomers from Queen's University Belfast have discovered the nature of five supernova precursor stars using Hubble images. The study reveals that stars with masses as low as seven times the mass of the Sun can explode as supernovae, challenging current understanding of massive star collapse.
Researchers found two star systems with yellow supergiant eclipsing binary characteristics, which may be the progenitors of rare supernovae. The discovery was made using the Large Binocular Telescope and suggests that these systems could explain the unusual nature of certain supernovae.
Researchers have discovered a neutron star that undergoes a dramatic transformation from a pulsar to a magnetar, providing insight into the evolutionary connection between these two types of ultradense objects. The discovery was made using data from NASA's Rossi X-ray Timing Explorer and Chandra X-ray Observatory satellites.
Astronomers have found a clue to the evolutionary relationship between pulsars and magnetars by examining archival RXTE data of a young neutron star. The study reveals that a regular pulsar can produce powerful bursts similar to those from magnetars, challenging current understanding of their life cycles.
Researchers using Chandra X-ray Observatory data have reported a possible detection of a binary star system that was later destroyed in a supernova explosion. The new method provides great promise for finding the detailed origin of these cosmic events.
Researchers suggest that unusual supernovae could confirm the existence of intermediate-mass black holes in globular clusters. The proposed mechanism involves tidal disruption of a white dwarf star by a black hole, causing explosive burning and a unique signature.
New research by Arecibo Observatory increases the mass limit for neutron star formation into black holes, suggesting they may be more rare. Neutron stars are found to remain stable between 1.9 and 2.7 sun masses, contradicting previous thought.
Two distinct gas and dust clouds formed by different types of supernova explosions are detected in DEM L316 nebula, with one shell containing more iron suggesting a Type Ia supernova. The two shells appear to be aligned by chance in the sky due to their vastly different ages.
A team of astronomers discovered that a white dwarf, AE Aquarii, emits high-energy X-rays as it whirls around on its axis, similar to the Crab Nebula's pulsar. This behavior indicates that white dwarfs can accelerate charged particles to near-light speed, potentially contributing to cosmic rays.
A team of researchers proposes a new mechanism to explain the brightest ever recorded supernova, SN 2006gy. The model suggests that an extremely massive star undergoes repeated explosions, resulting in a display up to 100 times more luminous than usual.
Astronomers study G292.0+1.8 supernova remnant to understand complex star death and dispersal of elements like oxygen into next generation of stars and planets. The new Chandra image shows an intricately structured debris field with varying temperatures, indicating lopsided explosion.
Astronomers have found an exceptionally massive black hole in orbit around a huge companion star in the nearby galaxy M33, with a mass of 15.7 times that of the Sun. The discovery raises questions about how such a big black hole could have formed.
Recent observations from NASA and Japanese X-ray observatories have helped clarify the origin of cosmic rays. The study, published in Nature, suggests that magnetic fields in supernova remnants are stronger than previously thought, enabling them to accelerate charged particles to enormous energies.
The National Research Council recommends pursuing the Joint Dark Energy Mission as the first mission in the 'Beyond Einstein' program, which aims to study dark energy. The report also suggests investing additional funds in technology development of the Laser Interferometer Space Antenna (LISA) program.
The National Research Council recommends the Joint Dark Energy Mission, supported by NASA and DOE, to study dark energy's role in the universe's expansion. The mission aims to map the sky with unprecedented resolution and study Type Ia supernovae to shed light on this mysterious entity.
Researchers from the Weizmann Institute of Science have observed a rare and detailed view of a Type Ia supernova event, revealing the remnants of a red giant star that fed a white dwarf. This unique observation supports a widely accepted model of these explosions.
Astronomers have identified Calvera, a bright X-ray source in Ursa Minor, as a promising candidate for an isolated neutron star, potentially the closest known. The team used NASA's Swift satellite and other telescopes to pinpoint its position and confirm its characteristics.
The Gruber Cosmology Prize has been awarded to Saul Perlmutter, Brian Schmidt, and their teams for discovering the accelerating expansion of the universe, dominated by mysterious dark energy. The breakthrough was made possible through innovative techniques using distant Type Ia supernovae as standard candles.
Researchers discovered clear changes in interstellar material absorption, indicating the existence of gaseous shells around a white dwarf. The system was likely composed of a white dwarf feeding on its red giant companion, leading to the supernova explosion. This finding strongly supports the Type Ia supernova scenario.
Astronomers have observed two Type II and Type Ia supernovae exploding in the same galaxy just 16 days apart. The rare event is unlikely to be related to anything unusual about the galaxy.
Astronomers have witnessed the death of a very massive star by observing two celestial explosions at exactly the same position in the sky. The most likely explanation for the 2004 explosion was a giant outburst of the star, which was later confirmed by the final death of the same star.
Astronomers can now compete for coordinated observing time on both GLAST and NRAO radio telescopes to study celestial objects in multiple wavelengths. This collaboration enables the study of flares from blazars, a key area of research to understanding supermassive black holes.
The star's mass is estimated at between 100 and 200 times that of the sun, making it one of the rarest types of massive stars. The supernova's brightness and longevity are attributed to its potential as a pair-instability supernova, which would produce a significant amount of heavy elements.
The MiniBooNE experiment resolves a long-standing question about neutrino behavior, contradicting earlier DOE findings. Researchers now push the search for sterile neutrinos with LENS project, potentially altering our understanding of particle physics.
Astronomers observed a massive star suffering a double whammy, with the star surviving one outburst before exploding as Supernova 2006jc. The study found that the supernova's blast wave interacted with material ejected by the star two years earlier, indicating a unique stellar evolution process.
Researchers have discovered that all Type Ia supernovae explode with the same mass and energy, making them useful for measuring distances. The brightness of supernovae depends on the amount of nickel they contain, allowing for more accurate calibration and future distance measurements.
Astronomer Nathan Smith proposes a new theory for the origin of the 1987 supernova's triple-ring nebula, suggesting that unstable blue supergiant stars, called luminous blue variables, may be responsible. Three nearby stars with similar nebulae have been discovered, contradicting the prevailing merger and red-to-blue transition explana...
A team of astronomers has solved the long-standing mystery of Kepler's supernova remnant using Chandra's latest image, revealing it as a Type Ia supernova. The discovery sheds light on how stars can end catastrophically and expands our understanding of the universe.
Researchers at the University of Illinois at Urbana-Champaign have observed a superbubble forming in the Small Magellanic Cloud, a galactic neighbor of the Milky Way. The study reveals that multiple massive stars are blowing bubbles and overlapping supernova remnants, which may eventually merge into one enormous cavity.
The University of Chicago's Center for Astrophysical Thermonuclear Flashes will perform the world's most advanced simulations of exploding white dwarf stars using 2.5 million hours of processing time. The goal is to understand the nature of dark energy, a mysterious force dominating the universe.
Recent gamma-ray bursts suggest a new kind of cosmic explosion involving newly formed black holes swallowing parent star matter. Astronomers observe no supernovae associated with these events, which could be due to massive stars dying without producing explosions.
Scientists have identified a new type of massive stellar death, where stars may collapse into black holes without exploding in supernova explosions. This discovery was made using data from two long-duration Gamma-ray bursts detected by NASA's Swift satellite.