Researchers discovered a previously unknown link between young star growth and black hole feeding habits, revealing the universality of accretion physics. The study found that young stellar objects' flickering light is similar to that of black holes and white dwarfs, supporting the idea that accretion is a universal process.
A team of astronomers at the University of Maryland and NASA's Goddard Space Flight Center has found evidence for a new intermediate-mass black hole about 5,000 times the mass of the sun. The discovery adds to the list of potential medium-sized black holes and strengthens the case for their existence.
Astronomers reanalyzed archival data to find only 11 galaxies with 'genuine' mergers, leading to a lower estimated rate of galaxy mergers and potentially fewer supermassive black hole pairs. This reduces the level of expected gravitational waves from X-shaped radio galaxies.
Astronomers at Columbia University provide evidence of a pair of supermassive black holes converging towards a collision. They predict the smashup will occur in 100,000 years, offering insights into black hole growth and space-time vibrations.
A University of Cincinnati study found that black voters are more likely to support black Democratic candidates, but may consider voting for a Republican candidate if they know the candidate's party affiliation. The study suggests that building a Republican coalition with black voters is challenging due to ongoing racial and partisan t...
A recent study published in Monthly Notices of the Royal Astronomical Society found that trained volunteers can identify jets shooting from massive black holes and match them to their host galaxies with high accuracy. The project, Radio Galaxy Zoo, uses online tutorials to teach volunteers how to spot black holes and other objects emit...
A team of astronomers discovered 48 Dust Obscured Galaxies (DOGs) using the Hyper Suprime-Cam instrument on the Subaru Telescope. These rare galaxies are thought to harbor rapidly growing black holes, providing insights into the co-evolution of galaxies and supermassive black holes.
A study by Florida Atlantic University finds that black borrowers, especially low-income black women, pay significantly higher interest rates on home mortgages compared to their white counterparts. The rate difference can be substantial, resulting in additional monthly mortgage payments and lost wealth over time.
Researchers discovered neutron stars can accelerate material to nearly light speed, rivaling black holes. This finding contradicts previous theories about neutron star behavior.
A recent study suggests that dense star clusters in the universe could be 'factories' of binary black holes. Researchers predict that advanced observatories will detect over 100 merging black holes per year from these clusters.
Astronomers have found a super-sized black hole in the early universe that grew faster than its host galaxy, challenging previous observations. The massive black hole, measuring 7 billion solar masses, is located in galaxy CID-947 and has a mass similar to that of a typical galaxy.
A team of researchers discovered a massive black hole with nearly 7 billion solar masses in an otherwise normal, distant galaxy called CID-947. The finding contradicts previous theories on the co-evolution of galaxies and their central black holes.
Astronomers detected high-energy x-rays from five previously clouded supermassive black holes, supporting the theory of millions more existing but hidden from view. The research uses NuSTAR to study nine candidate black holes, confirming five were obscured by dust and gas.
Researchers found strong outflows in ultra-luminous X-ray sources (ULXs), suggesting smaller black holes than expected. The team's observations shed light on ULXs and their impact on our understanding of supermassive black hole formation.
A new NASA simulation reveals that dark matter particles colliding in a black hole can produce strong, potentially observable gamma-ray light. This detection could provide new insights into both black holes and the nature of dark matter.
Astronomers using ALMA measured the mass of a supermassive black hole at the center of NGC 1097, a barred spiral galaxy 45 million light-years away. The black hole was found to be 140 million times more massive than our Sun.
The detection of a supermassive black hole at the center of Messier 32, a satellite of the Andromeda Galaxy, reveals a 'quiescent' black hole with activity among the weakest yet found. The VLA's improved sensitivity allowed for the detection of radio emission from the black hole, which is roughly 90 times fainter than previous studies.
Physicist Samir Mathur proposes that the surface of a black hole is not a fiery firewall but rather a benign copy machine creating an imperfect hologram. This idea counters the prevailing firewall theory and has significant implications for our understanding of the universe as a hologram.
A recent study by Omotayo Banjo found that black audiences are more comfortable watching black-oriented entertainment television with other black peers than with white counterparts. Black participants reported more positive excitement, attitudes, and absorption when viewing the program with all-black audiences. In contrast, white viewe...
Astronomers have combined telescopes across the Earth to create the Event Horizon Telescope, which will take detailed images of the supermassive black hole at the center of the Milky Way galaxy. The South Pole Telescope has joined the EHT, bringing a two-to-three times increase in resolution to study black holes and test Einstein's the...
Researchers found a pulsing quasar in the Pan-STARRS1 Medium Deep Survey, which could be evidence of a binary supermassive black hole system. The discovery sheds light on the end stages of galaxy mergers and may aid in pinpointing thousands of merging supermassive black holes.
Astronomers have detected strong magnetic fields near the event horizon of a supermassive black hole using ALMA. The findings provide new insights into the mysterious mechanisms driving jet formation, with magnetic fields playing a crucial role in matter escape.
Astronomers have detected an extremely powerful magnetic field close to a supermassive black hole in a distant galaxy, revolutionizing our understanding of these cosmic phenomena. The discovery was made using the Alma telescope and reveals new insights into the structure and formation of black holes.
Researchers at RIT studied binary spinning black hole interactions, revealing a long-term spin dynamic that continuously flips the spin until merger. This process may affect the growth of black holes surrounded by accretion disks and alter galactic and supermassive binary black holes.
New research shows that black holes do not erase information, but rather preserve it through the interactions of particles emitted by the black hole. This discovery challenges the long-standing 'information loss paradox' in physics.
A study by University of Maryland scientists has found a functional link between supermassive black holes and molecular outflows in galaxies. The research suggests that the black holes' winds are powerful enough to drive these massive outflows, which remove star-making gas and shape the galaxy's fate.
Researchers connect a black hole's 'wind' to an outward torrent of cold gas in a galaxy, validating feedback mechanisms that influence galaxy evolution. The discovery resolves a long-standing puzzle and sheds light on the relationship between supermassive black holes and their host galaxies.
The Canadian Space Agency has delivered its hardware contribution to the ASTRO-H mission, a flagship x-ray astronomy observatory. Professor Brian McNamara will study the effects of black holes on emergent galaxies, utilizing one of the most sensitive spectrometers in orbit.
A team of astronomers has found that galactic 'rain' may be the key to understanding why some galaxies are more productive at creating stars than others. The researchers analyzed X-rays from over 200 galaxy clusters using NASA's Chandra X-ray Observatory and discovered that massive black holes can slow down gas that helps form stars.
Astrophysicist Dr. Michael Kesden's research provides new insights into binary black hole mergers and their connection to gravitational wave detection. The solutions can significantly impact the study of black holes and the search for gravitational waves in the cosmos.
An international team of astronomers has found a huge and ancient black hole powering the brightest object in the early universe. The massive black hole is 12 billion times the size of our Sun and lives at the center of a quasar, emitting millions of billions of times more energy than the Sun.
Researchers detected a nearly spherical stream of highly ionized gas streaming out of the quasar PDS 456, measuring the strength of ultra-fast black hole winds. The discovery reveals that these powerful winds can transfer energy back to their host galaxies and affect star formation.
Researchers used computer code to generate images of wormholes and black holes, discovering multiple images of stars and galaxies near rapidly spinning black holes. This technology has implications for astrophysicists studying black holes and the behavior of light in extreme environments.
Researchers found black holes exist in gravitational theories with broken Lorentz invariance due to universal horizons, which prevent infinite speeds. Universal horizons act like cosmic boundaries that particles can move around but cannot escape, resolving a long-standing paradox.
Using supermassive black holes to measure cosmic distances provides precise distance measurements, removing uncertainty in calculating their mass. The new method shows that supermassive black holes are 40% heavier than previously estimated, fundamentally changing determinations of black hole masses.
Researchers have identified an enigmatic object named SDSS1133, which could be a recoiling black hole ejected from its parent galaxy. The discovery, made using high-precision equipment and observations with the Hubble Space Telescope, presents a unique opportunity to study gravitational waves and their detection.
Researchers at Cardiff University have built a theoretical model to predict potential gravitational-wave signals from black hole collisions. The model aims to help scientists identify the correct waveforms and reveal secrets about how black holes orbit and collide.
A team led by Andrea Ghez determined that G2 is most likely a pair of binary stars that had been orbiting the black hole in tandem and merged together into an extremely large star. The research suggests that many of the stars at the center of the galaxy are massive and mostly binaries.
Astronomers at Ohio State University have observed a star narrowly escaping capture by a supermassive black hole, releasing only a small portion of its mass. The event, known as a tidal disruption event (TDE), provides valuable insights into the growth and behavior of black holes in the universe.
Researchers at Johns Hopkins University found that massive black holes can block the formation of new stars in mature galaxies. The study suggests that these jets of radio-frequency feedback streaming from central black holes prevent hot gas from cooling and collapsing into baby stars.
Astronomers have discovered a pulsating, dead star beaming with the energy of about 10 million suns. Pulsars are dense stellar remnants leftover from supernovas, and this one is the brightest ever recorded.
Astronomers discovered a black hole named P13 that is consuming gas from a nearby star 10 times faster than previously thought possible. The black hole is ingesting a weight equivalent to 100 billion billion hot dogs every minute.
Astronomers using Hubble have found the smallest known galaxy with a supermassive black hole at its center. The galaxy, M60-UCD1, has a diameter of just 300 light-years and contains 140 million stars, yet it harbors a massive black hole weighing five times that of the Milky Way's central black hole.
Astronomers used Hubble and ground observations to find the M60-UCD1 dwarf galaxy containing a massive black hole. The discovery suggests compact galaxies may be remnants of larger galaxies torn apart during collisions.
Researchers found a tiny galaxy, M60-UCD1, hosting a supermassive black hole with a mass of 21 million suns. The discovery suggests many ultracompact dwarf galaxies may contain huge black holes. The team used Gemini North and Hubble Space Telescope observations to estimate the black hole's mass.
Researchers have found a supermassive black hole at the center of an ultra-compact galaxy, M60-UCD1, with a mass of 21 million suns. This discovery suggests that these massive black holes are more common in less-massive galaxies than previously thought.
New observations from NASA's Venus Express mission show giant holes in Venus' ionosphere, suggesting a more complex magnetic environment. The findings provide additional clues to understanding Venus' atmosphere and its interactions with the solar wind.
Researchers have identified an unusual midsize black hole called M82 X-1, measuring around 400 solar masses. The study analyzed six years of RXTE data to detect specific changes in brightness that helped determine the object's mass.
Astronomers have accurately measured a rare black hole about 400 times the mass of our sun in a galaxy 12 million light years from Earth. The finding confirms the existence of intermediate-mass black holes, which were previously disputed due to lack of data.
Researchers propose a solution for the rapid growth of ancient quasars, where small black holes zigzagged through dense gas streams, pulling in material and feeding on it rapidly. This mechanism allowed the black holes to grow at an exponential rate, eventually leading to massive growth rates.
Researchers from Moscow Institute of Physics and Technology have reported detecting three possible occasions of star destruction by supermassive black holes at galaxy centers. Using data from X-ray orbiting observatories ROSAT and XMM-Newton, they identified three X-ray sources with significant dimming, suggesting the death of a star i...
Astronomers have discovered three closely orbiting supermassive black holes in a galaxy over four billion light years away. The system's tight configuration suggests that these closely-packed black holes are far more common than previously thought.
An international team of astronomers discovered a clumpy gas stream flowing quickly outward and blocking 90 percent of the X-rays emitted by the supermassive black hole at the center of the galaxy NGC 5548. The researchers believe this activity provides new insights into the interaction of supermassive black holes and their host galaxies.
Researchers detected a clumpy gas stream flowing quickly outwards and blocking X-rays emitted by the supermassive black hole. The discovery provides direct evidence for the shielding process that accelerates powerful gas streams, offering insights into how black holes interact with their host galaxies.
An international team discovered that black hole outflows obscure observations and x-rays, shedding light on their impact on structure formation. The research provides a better understanding of these outflows and their role in regulating growth, using data from multiple space observatories.
A new study reveals magnetic fields near supermassive black holes can match the force of their gravitational pull, affecting gas dynamics and outflows. Magnetic field strengths are comparable to those produced by MRI machines.
Astronomers have found evidence that two classes of blazars represent different sides of the same cosmic coin, with one class being a gas-guzzling car and the other an energy-efficient electric vehicle. The team's redshift survey revealed that FSRQs began to decline while BL Lacs increased in numbers around 5.6 billion years ago.
Research by Princeton University graduate student David Pedulla found that negative stereotypes of gay men and black men can counteract each other for gay black men in employment, leading to higher starting salaries. This challenges the idea that membership in multiple marginalized groups leads to more discrimination.
Cosmic slurp: Researchers used NSF XSEDE supercomputers to simulate tidal disruptions of stars by supermassive black holes, predicting their observational signatures. This will help advance our understanding of galactic physics and properties of supermassive black holes.
A recent study by Rice University and colleagues analyzed the environmental fate of black carbon in deep ocean sediments. They found that more than half of black carbon never reaches the bottom, but instead stays dissolved in seawater or gets trapped in particles before sinking to the seafloor.