Researchers from Cardiff University found that the different tones of a dying black hole can provide insight into its mass and spin. By analyzing these tones, scientists may be able to weigh two black holes after they've collided and merged, potentially testing Einstein's general theory of relativity.
SourceCardiff University·JournalPhysical Review Letters·DateSep 17, 2012
Astronomers found a cloud of hydrogen and helium plunging toward the galactic center, which represents the remains of a planet-forming disk. The discovery suggests that planets can still form near black holes due to stars in a ring orbiting the galaxy's central black hole.
SourceCenter for Astrophysics | Harvard & Smithsonian·JournalNature·DateSep 11, 2012
The conference aimed to examine recent developments in active galactic nuclei and their effect on star formation. Researchers now believe that the energy released by supermassive black holes controls this process, which is crucial for galaxy evolution.
Astronomers have discovered galactic winds measuring up to 2,500 km/s, driven by intense bursts of star formation, potentially shutting down galaxy star formation. Young, compact galaxies with high-velocity winds are rare and may be part of a common phase in galaxy evolution.
SourceUniversity of California - San Diego·JournalThe Astrophysical Journal Letters·DateAug 20, 2012
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The Phoenix cluster holds the record for the fastest star formation rate in a galaxy cluster's center, breaking previous assumptions about cosmic evolution. The cluster's high star birth rate and rapid cooling of hot gas are expected to be short-lived due to unsustainable growth.
The Phoenix Cluster, discovered by the NSF's South Pole Telescope, is creating stars at an unprecedented rate of 20 times faster than in other clusters. The cluster's central galaxy and super-massive black hole are undergoing unsustainable growth, adding mass quickly before it becomes unsustainable.
SourceU.S. National Science Foundation·JournalNature·DateAug 15, 2012
Astronomers have discovered a massive galaxy cluster, known as the Phoenix Cluster, that is breaking several important cosmic records. Stars are forming in this object at the highest rate ever seen in the middle of a galaxy cluster.
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Researchers have identified a QPO signal in a distant galaxy's black hole, revealing insights into the nature of compact objects. The detection extends the reach of relativity testing to smaller black holes, about 3.5 minutes apart.
SourceNASA/Goddard Space Flight Center·JournalScience·DateAug 2, 2012
Intermediate-mass black holes can grow in galaxy gas disks through a mechanism similar to giant planet formation. The 'runaway growth' phenomenon allows stellar black holes to swallow stars and increase their mass, potentially creating an intermediate-mass black hole.
SourceAmerican Museum of Natural History·JournalMonthly Notices of the Royal Astronomical Society·DateJul 19, 2012
Researchers aim to achieve superconductivity at non-cryogenic temperatures by studying polariton condensates, a phenomenon exhibiting quantum collective behavior. Theoretical physicist Eric Bittner and experimentalist Carlos Silva will collaborate on the project.
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Astronomers have confirmed the first known 'middleweight' black hole, HLX-1, using observations with CSIRO's Australia Telescope Compact Array. The black hole is estimated to be around 20,000 to 90,000 times the mass of the Sun and lies in a galaxy called ESO 243-49.
New study finds that most massive black-hole growth in the early universe was fueled by small, long-term events rather than dramatic short-term major mergers. Quasars thrive in normal-looking spiral galaxies, triggered by black holes snacking on gas or small satellite galaxies.
Researchers suggest that axions, hypothetical particles with low mass, could accumulate around black holes and emit gravity waves. This process could be measured using existing detectors, providing insights into astronomy and potentially revealing new particle types.
SourceVienna University of Technology·JournalPhysical Review D·DateJun 18, 2012
A new study using Chandra data reveals two galaxies with supermassive black holes growing at a rate outpacing their host galaxies. The findings suggest that dark matter halos and black holes are linked in the growth of these galaxies, contradicting previous assumptions.
Astronomers use XMM-Newton data to detect X-ray 'echoes' from a distant galaxy, revealing a new way to study supersized black holes and their accretion disks. The echoes, which lag behind AGN flares by up to 30 minutes, provide insights into the environment around these massive black holes.
SourceNASA/Goddard Space Flight Center·JournalMonthly Notices of the Royal Astronomical Society·DateMay 31, 2012
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Astronomers using Herschel Space Observatory data show that massive black holes at galaxy centers influence star formation rates. Galaxies with powerful black holes form stars at a thousand times the rate of Milky Way, but fastest-growing black holes shut off star formation in surrounding galaxies.
Astronomers have discovered a supermassive black hole eating a star's core, revealing that these massive objects snack infrequently. The discovery showcases the power of the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) in detecting transient phenomena.
SourceCenter for Astrophysics | Harvard & Smithsonian·JournalNature·DateMay 3, 2012
Astronomers at Queen's University Belfast have gathered direct evidence of a supermassive black hole shredding a star that wandered too close. The discovery provides insights into the harsh environment around black holes and the types of stars swirling around them.
SourceQueen's University Belfast·JournalNature·DateMay 3, 2012
Astronomers have gathered direct evidence of a supermassive black hole ripping apart a star that strayed too close. The team identified the victim as a helium-rich star in a galaxy 2.7 billion light-years away, providing insights into the harsh environment around black holes.
SourceNASA/Goddard Space Flight Center·JournalNature·DateMay 2, 2012
A team of astronomers led by Suvi Gezari has identified a star rich in helium gas that was ripped apart by the gravitational forces of a supermassive black hole. The star's remains were seen falling into the black hole, while the rest was ejected at high speeds, providing insights into the harsh environment around black holes.
SourceJohns Hopkins University·JournalNature·DateMay 2, 2012
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Astronomers have discovered a group of over 675 hypervelocity stars on the outskirts of the Milky Way, which are believed to have been ejected from the galactic core. These stars, found in intergalactic space between the Milky Way and Andromeda galaxy, exhibit high metallicity indicating an inner galactic origin.
The IceCube Collaboration found no evidence of ultra-high-energy cosmic rays originating from gamma-ray bursts, challenging the long-held theory. Instead, the team suggests that active galactic nuclei may be responsible for accelerating these particles.
SourceDOE/Lawrence Berkeley National Laboratory·JournalNature·DateApr 18, 2012
Australians and Koreans have linked their radio telescopes for the first time, creating a gigantic telescope spanning over 8,000 km. The combined system has 100 times the resolving power of the Hubble Space Telescope, enabling scientists to study distant galaxies in unprecedented detail.
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The closest large elliptical galaxy to the Milky Way, Centaurus A has a twisted disc of dust near its centre, formed from a cosmic collision with another galaxy. The galaxy's powerful heart features two massive jets streaming from a massive black hole, emitting strong radio emission and visible in far-infrared images.
SourceUK Space Agency·JournalMonthly Notices of the Royal Astronomical Society·DateApr 4, 2012
New research reveals that supermassive black holes can double in mass by ripping apart double-star systems and swallowing one of the stars. This process is thought to be the dominant method for growing these massive objects.
SourceCenter for Astrophysics | Harvard & Smithsonian·JournalThe Astrophysical Journal Letters·DateApr 2, 2012
A University of Utah astrophysicist has proposed that supermassive black holes in galaxy centers grow by consuming single stars from wandering binary pairs. The study found that this process is an efficient way to bring stars close to black holes, outperforming gas clouds as a growth mechanism.
SourceUniversity of Utah·JournalThe Astrophysical Journal Letters·DateApr 1, 2012
Researchers have identified hypervelocity planets and stars that are ejected from the Milky Way at millions of miles per hour due to their close interaction with a massive black hole. The study suggests that these high-speed objects can provide valuable insights into planetary formation and evolution near the central black hole.
SourceDartmouth College·JournalMonthly Notices of the Royal Astronomical Society·DateMar 29, 2012
Researchers suggest that highly massive black holes began growing rapidly in the early universe due to chaotic gas flows. By simulating gas discs orbiting a black hole at different angles, they found that collisions between these discs can lead to a significant increase in the black hole's mass.
SourceUniversity of Leicester·JournalMonthly Notices of the Royal Astronomical Society·DateMar 23, 2012
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Astronomers have identified a new type of black-hole-driven outflow that explains the link between galaxy mass and star velocity. Ultra-fast outflows are common features of black-hole-powered galaxies, influencing galactic shape and star formation.
SourceNASA/Goddard Space Flight Center·JournalMonthly Notices of the Royal Astronomical Society·DateFeb 27, 2012
Astronomers have discovered a young cluster of blue stars surrounding an intermediate-mass black hole in a cannibal galaxy. The star cluster is thought to be less than 200 million years old and may be the remnant of a dwarf galaxy that was swallowed by the larger galaxy.
Researchers found a cluster of young, blue stars encircling the first intermediate-mass black hole ever discovered in a dwarf galaxy. The presence of this star cluster suggests that the black hole was once at the core of the now-disintegrated dwarf galaxy.
SourceCenter for Astrophysics | Harvard & Smithsonian·JournalThe Astrophysical Journal Letters·DateFeb 15, 2012
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The study suggests a massive cloud of trillions of asteroids and comets surrounds Sgr A*, where they are vaporized by friction as they pass through the hot gas flowing onto the black hole. The flares observed by Chandra could be explained by the frequent collision of asteroids with the black hole.
SourceChandra X-ray Center·JournalMonthly Notices of the Royal Astronomical Society·DateFeb 8, 2012
The Hubble Space Telescope has created the sharpest visible-light image ever made of the nucleus of an external galaxy, the Andromeda galaxy. The blue stars surrounding the massive black hole are just 200 million years old and formed in a burst of star formation near the black hole.
An international team of astronomers identified the moment when a black hole launched super-fast knots of gas into space using NASA's RXTE and NSF's VLBA radio telescope. The 'bullets' of ionized gas were thought to arise from a region outside the event horizon, where they were associated with changes signaling the start of the process.
Researchers used the VLBA and RXTE satellite to study a 2009 outburst from a black hole system. The collaboration gathered detailed images of
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Astronomers will use a new telescope called X-Calibur to study the polarization of X-rays, providing information about cosmic sources that is not available elsewhere. The instrument will be sensitive to hard X-rays and will be flown at an altitude of 40 kilometers, allowing it to focus on celestial objects with high accuracy.
SourceWashington University in St. Louis·DateJan 6, 2012
Astronomers identify smallest-known black hole using data from NASA's Rossi X-ray Timing Explorer (RXTE). The 'heartbeat' pattern, similar to an electrocardiogram, suggests a minuscule black hole weighing less than three times the sun's mass.
SourceNASA/Goddard Space Flight Center·JournalThe Astrophysical Journal Letters·DateDec 15, 2011
Astronomers have discovered a unique new object, a dusty ionized gas cloud, nearly doubling its speed in seven years and approaching the event horizon of the black hole. The cloud will break apart completely over the next few years due to external pressure and gravitational pull.
Astronomers are observing a unique opportunity to study how a black hole gulps gas, dust, and stars as it grows bigger. The gas cloud is currently 550 Kelvin or 280 degrees Celsius and will be ripped apart by the tidal forces around the black hole.
SourceUniversity of California - Berkeley·JournalNature·DateDec 14, 2011
Researchers have discovered two massive black holes, each with a mass equivalent to 10 billion suns, in nearby galaxies. These 'sleeping giants' are thought to be remnants of quasars that powered the early universe.
SourceU.S. National Science Foundation·JournalNature·DateDec 12, 2011
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Researchers recreated universe's first billion years using largest cosmological simulation to date. Thin streams of cold gas flowed into early black holes, causing rapid growth and challenging astrophysical theory.
SourceCarnegie Mellon University·JournalThe Astrophysical Journal Letters·DateDec 12, 2011
Astronomers have found two massive black holes, each with a mass of 10 billion suns, in nearby galaxies. These 'sleeping giants' are thought to be remnants of quasars that powered matter into black holes in the early universe.
SourceU.S. National Science Foundation·JournalNature·DateDec 6, 2011
Astronomers have discovered the largest black holes to date, two monsters with masses equivalent to 10 billion suns threatening to consume anything within a region five times the size of our solar system. These black holes are located in giant elliptical galaxies more than 300 million light years from Earth.
SourceUniversity of California - Berkeley·JournalNature·DateDec 5, 2011
Astronomers have discovered two gigantic black holes with masses about 10 billion times the mass of our sun, surpassing previous measurements by more than 50 per cent. The discovery suggests that these massive black holes may be the dormant remains of extremely luminous quasars from billions of years ago.
SourceUniversity of Toronto·JournalNature·DateDec 5, 2011
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For the first time, astronomers have produced a complete description of a black hole using precise measurements. The new information reveals that the black hole is nearly 15 times more massive than our Sun and spinning over 800 times per second.
SourceNational Radio Astronomy Observatory·JournalThe Astrophysical Journal Letters·DateNov 17, 2011
A new theory suggests that high-speed collisions between planets and asteroids near supermassive black holes create microscopic dust clouds. This process blocks harmful radiation, creating a more hospitable environment for life in the galaxy's central region.
SourceUniversity of Leicester·JournalMonthly Notices of the Royal Astronomical Society·DateOct 28, 2011
Researchers at Princeton University and NYU have developed a method to detect the collision of stars with primordial black holes, which are believed to be a source of dark matter. The new technique uses existing solar observation methods to identify subtle vibrations in a star's surface caused by a passing black hole.
SourcePrinceton University·JournalPhysical Review Letters·DateSep 19, 2011
Astronomers have found supermassive black holes in small distant galaxies, suggesting that central black holes formed early in galaxy evolution. The study used the Hubble Space Telescope to probe the universe and identifies a connection between star formation and active galactic nuclei.
SourceUniversity of California - Santa Cruz·DateSep 15, 2011
Astronomers have discovered a unique spiral galaxy with massive jets, providing insights into the formation of galaxies and clusters in the early universe. The galaxy, dubbed Speca, has been found to exhibit three distinct episodes of jet activity, shedding new light on the processes that shaped these ancient structures.
SourceNational Radio Astronomy Observatory·JournalMonthly Notices of the Royal Astronomical Society·DateAug 25, 2011
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Two studies reveal that the star was torn apart by intense tides as it approached the black hole, creating an unprecedented outburst of energy. The outburst produced X-rays and radio emissions that pointed straight at Earth, offering insights into relativistic beaming.
SourceNASA/Goddard Space Flight Center·JournalNature·DateAug 24, 2011
New research by University of York scientists proposes that quantum mechanics could be the key to understanding how black holes work, potentially allowing information to escape. The study's findings suggest a possible breakthrough in our understanding of gravity and its relationship with space and time.
SourceUniversity of York·JournalPhysical Review Letters·DateAug 10, 2011
Researchers detected massive water vapor in a distant quasar, equivalent to 34 billion times the mass of Earth. The discovery was made using a spectrograph called Z-Spec and reveals a time when the universe was only 1.6 billion years old.
SourceUniversity of Colorado at Boulder·JournalThe Astrophysical Journal Letters·DateJul 22, 2011
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Astronomers have discovered a massive reservoir of water vapor 30 billion light-years away in a quasar, which is 100,000 times more massive than the sun. The water vapor is distributed around a black hole and provides insights into its environment.
SourceCalifornia Institute of Technology·JournalThe Astrophysical Journal Letters·DateJul 22, 2011
Astronomers have found the largest and farthest reservoir of water ever detected in the universe, located in a distant quasar with a massive black hole. The discovery provides valuable information about the early universe's water vapor behavior and its influence on cosmic evolution.
SourceCarnegie Institution for Science·JournalThe Astrophysical Journal Letters·DateJul 22, 2011
A new study by Brigham Young University researchers reveals that black holes' movement, including lateral motion and spin, fuels massive jets of energy known as quasars. The study confirms a long-held theory while introducing a new component: that black holes' lateral movement also powers these jets.
SourceBrigham Young University·JournalProceedings of the National Academy of Sciences·DateJul 20, 2011
Scientists have discovered the most distant quasar to date, ULAS J1120+0641, with a redshift of 7.1, providing a unique opportunity to study the early universe. The object's massive black hole is estimated to be two billion times that of our Sun, challenging current theories on its growth.
SourceUniversity of Nottingham·JournalNature·DateJun 29, 2011
Astronomers discovered a massive black hole in a distant galaxy that ripped apart a star, creating a powerful beam of energy that crossed 3.8 billion light years to Earth. The extreme brightness of this event was due to the small fraction of the sky illuminated by the jet of light towards the Milky Way.
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A gamma-ray flash was detected coming from a distant galaxy, suggesting a massive black hole is consuming a star. The long-duration event produced an enormous amount of energy and appears to be emanating from the center of the galaxy.
SourceUniversity of California - Berkeley·JournalScience·DateJun 16, 2011
A Rutgers University astrophysicist's research team has discovered that supermassive black holes were surprisingly common in the early universe, growing at a rate similar to their host galaxies. The findings suggest there are at least 30 million black holes in the early universe, far exceeding previous estimates.
Researchers detected 13 billion light-year-old galaxies with hidden central black holes using the Chandra X-Ray Observatory. The findings suggest a symbiotic relationship between black holes and galaxies dating back to the Big Bang.