Articles tagged with Black Holes
The Fermi Gamma-ray Space Telescope has detected high-energy gamma-rays from the enigmatic binary system Cygnus X-3, a genuine microquasar. The system's unique properties and strong emission across various wavelengths offer new insights into how high-energy particles are accelerated and move through jets.
A new study led by CU-Boulder suggests that the first large black holes in the universe formed and grew inside gigantic, starlike cocoons. These cocoons likely prevented surrounding gases from being blown away and smothered powerful x-ray radiation.
Astronomers have found a middleweight black hole in galaxy NGC 5408, with masses between 1,000 and 9,000 solar masses. The discovery was made using the Swift satellite and XMM-Newton observatory, which detected quasi-periodic oscillations from the black hole.
Researchers at RIT are using supercomputers to study the massive dark objects, simulating what cannot be seen directly. The grants and allocations will enhance their access to sophisticated computer power, staying at the forefront of scientific computation.
The mosaic image reveals stellar evolution, bright young stars, and a supermassive black hole at the Galactic center. Giant X-ray flares from Sgr A* have occurred about 50 and 300 years earlier.
Mathematicians at the University of Leeds propose that black holes are directly responsible for producing gamma ray bursts, contradicting the orthodox model. The theory suggests that rotating black holes can devour nearby stars, creating long-lasting jets of plasma that produce the high-energy radiation.
A team led by Professor Stephen Eikenberry captured the first images of the cosmos using a UF-designed camera/spectrometer attached to the Gemini South telescope in Chile. The instrument, FLAMINGOS-2, will enable accurate tracking of black hole growth and evolution over 4 billion years.
Astronomers have discovered a giant galaxy surrounding the most distant black hole ever found, 12.8 billion light-years from Earth. The galaxy is as large as the Milky Way and harbors a supermassive black hole with at least a billion times more matter than our sun.
Dartmouth researchers have proposed a new method to create tiny quantum-sized black holes in the laboratory, allowing for better understanding of Hawking radiation. The SQUID-based setup enables exploration of analogue quantum gravitational effects and may be more straightforward for detecting Hawking radiation.
A NASA/Goddard Space Flight Center simulation found that the universe's first black holes grew slowly due to a lack of gas, contrary to expectations. The findings have significant implications for understanding galaxy formation and the role of black holes in shaping the universe.
Recent simulations by astrophysicists reveal that the first black holes in the universe grew slowly and were deprived of gas, contradicting popular theories. The simulations suggest that these early black holes may have played a more complex role in the formation of supermassive black holes observed today.
Researchers, including Dr. Dentcho Genov, successfully mimicked celestial mechanics using artificial optic materials to study phenomena around black holes and other celestial objects. The team's work has implications for technology, such as the 'invisibility cloak,' and confirms Louisiana Tech's contribution to vital science discoveries.
Researchers found that turbulence created by material ejected from supermassive black holes' disks prevents cooling gas from forming stars. The discovery explains a long-standing mystery in galaxy cluster physics.
Using a worldwide VLBA collaboration, scientists pinpoint the origin of superenergetic gamma rays coming from M87's core near the supermassive black hole. The discovery sheds light on the mechanisms powering galaxies' energetic jets.
Researchers have located the site of relativistic particle acceleration in galaxy M 87, where particles are accelerated to extreme energies and emit gamma rays with trillion-electron Volt energies. The discovery was made possible by combining high-resolution radio and gamma-ray observations using three arrays of telescopes.
A new class of black hole has been discovered, with masses between 100 and several hundred thousand times that of the Sun. The discovery, made by an international team of astronomers using XMM-Newton observations, confirms the existence of intermediate mass black holes.
A Kansas State University professor is studying new theories about the origin and future of life in the universe. He suggests that artificial black holes could play a part in the evolution of life and potentially spread it throughout the galaxy.
Astronomers at the University of Warwick have discovered that the 2006 stellar explosion SCP 06F6 bears remarkable resemblance to extremely carbon-rich stars. The object's unusual characteristics suggest it may be a new type of supernova, with properties distinct from normal Type II supernovae.
Astronomers observe a high-energy apparition, known as an X-ray ghost, lingering around a supermassive black hole in the Chandra Deep Field-North. The source, HDF 130, is 10 billion light years away and existed 3 billion years after the Big Bang.
Using XMM-Newton's new data, astronomers have mapped the region around a supermassive black hole, estimating its mass at 3-5 million solar masses. The observations also reveal rapid spinning and accretion rates that verge on theoretical limits.
New calculations suggest hundreds of massive rogue black holes are left over from the early universe, potentially wandering the Milky Way's outer reaches. These relics could provide clues about galaxy formation history and the formation of black holes in the early universe.
Researchers discovered a mechanism for regulating the rate at which stellar-mass black holes grow, suggesting that they can regulate themselves. The study found that the black hole in GRS 1915+105 toggles between expelling mass via a jet and a wind from its accretion disk.
Scientists have directly observed a gigantic star blowing up, supporting the idea that massive stars end as black holes. The explosion revealed most of the star's mass collapsed into a dense core, creating an invisible black hole.
The Sherman Fairchild Foundation has awarded $3.1 million to Caltech to support the SXS program, which simulates black hole collisions and neutron star ruptures with high accuracy using the Spectral Einstein Code (SpEC). The grant will enable the team to perfect SpEC and simulate other warped-spacetime phenomena.
Researchers have discovered a new connection between Carter's constant and Newtonian gravity, shedding light on the behavior of rotating black holes. The findings have significant implications for gravitational-wave astronomy, potentially allowing the detection of small black hole orbits.
Sandra Faber is being honored for her extraordinary advances in understanding the properties of distant galaxies, dark matter, large-scale structure, and black holes. Her innovative leadership has driven significant discoveries in modern cosmology, including the role of dark matter in galaxy formation.
Researchers harness supercomputing to recreate how galaxies form, develop, and collapse. The most detailed recreation of the universe's evolution to date is created using computer simulations that incorporate black hole physics.
The AAS High Energy Astrophysics Division has awarded the 2009 Rossi Prize to Charles D. Bailyn, Jeffrey E. McClintock, and Ronald A. Remillard for their work on measuring black hole masses in binary pairs with companion stars.
A team of Yale University astronomers discovered that galaxies stop forming stars before their central supermassive black holes reach their most powerful stage. The study found no bright AGN at the centers of star-forming galaxies, suggesting that the shutting-down process occurs earlier in the AGN's lifetime.
Astronomers are discovering that galaxies with actively forming stars have a bluish color, while those without do so appear red. The BAT Hard X-ray Survey of NASA's Swift spacecraft has found most nearby active galaxies to be spiral and irregular, with more than 30% being colliding.
A recent study suggests that supermassive black holes formed first and grew before their host galaxies. The ratio of black hole mass to galactic bulge mass is nearly constant across different galaxy sizes and ages. This finding implies that the growth of black holes and galaxies was an interactive process.
Researchers identified two protostars located just a few light-years from the Milky Way's central black hole, defying expectations that gravitational tides would prevent star formation. The discovery suggests molecular gas at the galactic center is denser than previously thought, allowing it to form new stars.
Astronomers use gravitational lensing effect to magnify light from quasar MG J0414+0534, detecting water vapour at redshift 2.64, a time when the Universe was only a fifth of its current age
Researchers found that all active galactic nuclei have a similar physical structure, independent of the black hole's size. The observation constrains current ideas on how glow around black holes is produced, allowing for further study of these enigmatic objects.
Researchers have discovered two distant galaxies with massive black holes at their centers, challenging previous assumptions about the formation of these cosmic objects. The study reveals that these colossal black holes were present even 12 billion years ago, when the universe was just 1.7 billion years old.
Astronomers have found that magnetic fields are essential for black holes to swallow matter. The variations in visible light and X-rays were found to follow a repeated pattern, indicating that strong magnetic fields store energy near the black hole.
Andrea Ghez, a UCLA professor of physics and astronomy, has been selected as a MacArthur Fellow for her pioneering work on supermassive black holes and their role in shaping the evolution of galaxies. Her research has improved our understanding of these enigmatic objects and shed light on their impact on the surrounding environment.
Researchers at Durham University found a giant black hole emitting a regular X-ray signal, linking it to smaller black holes. This discovery sheds light on how gas behaves around super-massive black holes as they feed and develop.
A Yale University astrophysicist has discovered an upper mass limit for black holes, which appear to curb their growth at around 10 billion times the mass of our Sun. This finding has implications for the study of galaxy formation and suggests that black holes may play a key role in regulating star formation.
Researchers used VLBI technique to combine signals from multiple telescopes and detected structure 30 million miles away from the galactic center. The observations provide unprecedented view of the region near the black hole event horizon.
A team of astronomers has obtained the closest views ever of a super-massive black hole at the center of the Milky Way galaxy. The new observations revealed the highest density yet for the concentration of matter at the galaxy's center, supporting the existence of black holes.
The Hubble Space Telescope has resolved individual threads of gas in the filaments of galaxy NGC 1275, revealing a magnetic structure that sustains them for over 100 million years. The discovery provides crucial clues about how giant black holes affect their surroundings.
A team of Caltech astronomers reveals that spiral galaxies have more bars than previously thought, with most forming in smaller, low-mass galaxies. The study suggests that bars play a crucial role in galaxy evolution, fueling new star formation and feeding massive black holes.
Researchers have successfully visualized the elusive disks of matter surrounding supermassive black holes using a polarising filter on the UK Infrared Telescope. This breakthrough allows scientists to study these black holes in greater detail, shedding light on their structure and composition.
Researchers have used radio telescopes to study the behavior of Seyfert galaxies, revealing that the majority of them are being consumed by black holes due to interactions with neighboring galaxies. This discovery provides strong evidence for the role of galactic cannibalism in powering these galaxies.
Dr. Joan M. Centrella and Dr. John G. Baker received the John C. Lindsay Memorial Award for their pioneering computer simulations of black hole mergers, a crucial step towards understanding cosmic evolution. The simulations have spurred rapid progress in predicting observable signatures of these events.
Maarten Schmidt's discovery of high redshifts in quasar 3C273 led to a new understanding of quasars as compact halos surrounding massive black holes. He shares the award with Donald Lynden-Bell for their contributions to astrophysics.
The Gamma-ray Large Area Space Telescope (GLAST) will search for answers to long-standing questions about dark matter, black holes, and gamma-ray bursts. With its extraordinary sensitivity and wide field-of-view, GLAST has the potential to detect thousands of hitherto unknown gamma-ray sources.
Researchers at Penn State have discovered a mechanism that allows information to be recovered from black holes, contrary to Stephen Hawking's previous assertion. By expanding space-time beyond its assumed size, the team finds room for information to reappear in the distant future.
Astronomers used VLBA to watch material winding a corkscrew path and confirm twisted magnetic fields accelerate particles. The team observed BL Lac, a blazar, with unprecedented view of the innermost portion of its jet.
A team of Japanese astronomers has discovered that the Milky Way's central black hole, Sagittarius A*, let loose a powerful flare three centuries ago. The finding resolves a long-standing mystery about the black hole's quiescent nature.
A RIT team successfully simulated the merger of three black holes, confirming a robust computer code and predicting distinct gravitational signatures. The simulation, which uses high-performance computing, is essential for detecting gravity waves that may confirm the existence of black holes.
Researchers have created an online map that shows locations experiencing problems with internet connectivity, providing a snapshot of the internet's weak points. The Hubble tool monitors about 90% of the internet and can help professional network operators identify and fix issues quickly.
Researchers used XMM-Newton to observe four polar BAL quasars, finding two of them emitted more X-rays than anticipated, suggesting a lack of absorbing gas. This discovery may indicate that BAL quasars are more complex than initially thought, with both equatorial and polar outflows potentially occurring simultaneously.
Astronomers have identified the smallest known black hole, with a mass of 3.8 times that of our Sun and a diameter of just 15 miles. The black hole resides in a binary system in the Milky Way Galaxy and was measured using archival data from NASA's Rossi X-ray Timing Explorer satellite.
The Virginia Tech group is exploring the possibility of an extra dimension, curled up like the universe at the Big Bang. They plan to detect small primordial black holes that produce radio pulses using a new Transient Array radio telescope.
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.
Astronomers have determined that a hyperfast star, HE 0437-5439, originated from the Large Magellanic Cloud, contradicting its initial assumption of coming from the Milky Way. The star's elemental composition and velocity indicate it was ejected from the LMC by a massive black hole.
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.
Researchers found that rapidly spinning black holes produce light echoes, where X-ray photons travel different paths around the black hole, causing a constant delay independent of source position. This effect would allow astronomers to measure black hole masses with high accuracy.