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.
Research by NSW DPI has identified the Whitefringed weevil larvae as the culprit behind small holes in leaky irrigation pipes. The larvae can chew through plastic piping using their dark brown pincers, leading to significant yield loss and water waste for lucerne growers.
Researchers found a strong correlation between black hole presence and reduced star formation in heavy galaxies. The energy generated by massive black holes may heat up gas, preventing new stars from forming.
Duke University researchers have devised a method to test for the presence of naked singularities, potentially existing in certain instances. Their study suggests that high-spin black holes could shed their event horizon and become observable through gravitational lensing effects.
A heat-sensitive camera has discovered seven small, deep holes on the flanks of Arsia Mons, a giant volcano on Mars. The team suggests that these holes may be openings to underground caves, formed as faults created stresses that opened spaces underground.
A new study using Chandra finds that younger, more distant galaxy clusters contain far more actively growing supermassive black holes than older, nearby ones. This rapid growth allows these black holes to thrive and influence their host galaxies.
The BHCosmo simulation reveals the integral role of black holes in galaxy formation and cosmic evolution. It provides a deeper understanding of quasar formation and helps predict where to aim future telescopes for early cosmic events and galaxy structures.
The discovery reveals how efficient neutron stars can be as cosmic power factories and shows they rival black holes in generating powerful jets. The X-ray jet is found to be almost as efficient as one from a black hole, with a surprising high percentage of energy converted into powering the jet.
Physicists Tanmay Vachaspati, Dejan Stojkovic, and Lawrence M. Krauss propose a solution to the long-standing problem of information loss in black holes. They suggest that non-thermal radiation can carry information about collapsing matter beyond the event horizon.
Scientists at RIT have discovered that supermassive black holes can be thrown from galaxies at speeds of up to 4,000 km/s, significantly exceeding the escape velocity. The spin velocity determines the size and direction of the 'kick' or radiation recoil.
Astronomers have used adaptive optics technology to pinpoint two supermassive black holes in a colliding galaxy. The observations reveal the black holes reside at the center of rotating disks of stars and are surrounded by young star clusters.
Researchers used adaptive optics to precisely locate and study the environments of two supermassive black holes at the center of a galaxy merger. The observations revealed young star clusters and rotating disks of stars surrounding each black hole.
Researchers discovered the location and makeup of a pair of supermassive black holes in a galaxy collision, using adaptive optics to clear atmospheric distortion. The discovery sheds light on the coevolution of black holes and galaxies, with implications for understanding galaxy evolution and properties.
Researchers have successfully applied a new method to determine the masses of black holes in binary systems, including Cygnus X-1 and NGC 5408. The technique takes advantage of X-ray observations of quasi-periodic oscillations (QPOs) and their relationship with the accretion disk.
Researchers at UC-San Diego have discovered that nanowire photodetectors can achieve single-photon sensitivity, making them highly sensitive to light detection. The unique geometry of nanowires traps holes, increasing the time electrons travel down the wire and triggering an increase in current.
Scientists confirm size of hot gas disk around supermassive black hole, measuring its size as seven times the distance between Earth and Sun. The disk is found to be 10 times smaller than predicted event horizon, consistent with theoretical predictions.
Astronomers found a trio of supermassive black holes in the Virgo constellation, 10.5 billion light-years away, with same redshift and distinct properties, raising questions about galaxy interactions and fundamental relationships between galaxies and black holes.
Researchers found that quasars with large black holes are more variable than those with low black hole masses, changing brightness by up to 15% over a year. The study's findings provide new insights into the physics behind quasar variability and could help astronomers decipher underlying mechanisms.
Scientists have discovered a supermassive black hole at the heart of a dwarf elliptical galaxy, VCC128, located 54 million light years away. The finding is significant as it shows that even small galaxies can host massive black holes, challenging previous assumptions.
A new study found that Black Caribbean immigrants in the US experience poorer mental health as they stay longer, with higher rates of mood and anxiety disorders among men and lower rates among women compared to African Americans. Third-generation immigrants had the highest disorder rates.
Astronomers found that black holes of all sizes follow the same 'feeding' process, with characteristic timescales changing linearly with mass and inversely with accretion rate. This discovery helps determine black hole masses in hard-to-reach cases.
Scientists have detected loops and rings of hot gas surrounding the supermassive black hole, indicating periodic eruptions that generate pressure waves and sound. The sound waves are found to be more discordant and complex than previously detected, with a range of frequencies below middle C.
For the first time, astronomers have looked inside quasars and seen evidence of black holes. They measured the size of the accretion disk around a smaller area emitting X-rays, providing further confirmation that quasars are made up of super-massive black holes and heated disks.
Astronomers are using supercomputers to study the energy levels of high-temperature atoms in space, which hold the key to understanding black holes. The new calculations reduce error rates by a few percent, providing more accurate data for X-ray telescope observations.
New X-ray data from Chandra reveals that magnetic fields are responsible for the prodigious amounts of radiation emitted by super-massive black holes. The discovery uses a scale model in our galaxy to understand how all black holes work, including those powering quasars.
Researchers found that defendants rated as 'stereotypically black' were sentenced to death at a rate of 57.5%, compared to 24.4% for those less stereotypically black, in cases involving white victims. However, this effect disappeared in 'black-on-black' capital cases.
Researchers predict that braneworld black holes, created in the early universe, have survived and can be detected by observing gamma-ray bursts passing near them. The signature of these black holes could provide evidence for a fourth dimension of space.
Black holes are surprisingly efficient at producing energy, with most of the energy released by matter falling toward a supermassive black hole going into high-energy jets. The study also shows that these jets create huge bubbles in the hot gas of galaxies, preventing new stars from forming.
Researchers have discovered a large number of supermassive black holes, outnumbering initial estimates, using deep X-ray surveys. The findings suggest that these black holes are more stable over time than previously thought.
A study found that only 25% of high-risk black men aged 60-69 are screened for prostate cancer, compared to 81% of white men. This disparity highlights a need for increased awareness and targeted screening efforts among black males with positive family histories.
A team from MIT and Harvard found that a certain type of X-ray explosion common on neutron stars is never seen around their black hole cousins, indicating the presence of an event horizon. The absence of surface explosions called X-ray bursts suggests that gas released by nearby stars vanishes into a void.
Two new studies using Hubble Ultra Deep Field data show a link between galaxy assembly and supermassive black hole growth. Tadpole galaxies, with bright knots and tails caused by mergers, suggest that black holes are enshrouded in dust, making them invisible during the merging process.
Astronomers have discovered that massive clouds of hot gas in elliptical galaxies are being stirred up by intermittent explosive activity from central super-massive black holes. This finding challenges the long-held assumption that these galaxies are quiet and stable, revealing a more dynamic and stormy reality.
A team of researchers from UCLA has discovered a group of over 30 young stars near a supermassive black hole, contradicting the idea that such an environment should prevent star formation. The stars' orbits suggest they formed in a massive star cluster and migrated towards the black hole.
UI researchers discovered a giant star orbiting a 'medium-sized' black hole every 62 days, indicating the star's enormous size and brightness in X-rays. This finding may help confirm a class of black holes with masses between 100 and 10,000 solar masses.
Astronomers find a dense whirling ball of neutrons in an extremely young star cluster, challenging the idea that nature can make black holes. The discovery shows massive stars may not collapse into black holes as predicted, but instead create neutron stars with a greater influence on future generations of stars.
Astronomers find massive stars forming close to super-massive black holes, challenging previous theories about their role in galaxy evolution. Researchers used Chandra X-ray Observatory data to study the Sagittarius A* (Sgr A*) star cluster near the Milky Way's central black hole.
Astronomers detect unusual quasar with no visible host galaxy, sparking debate about its origin. The object's properties suggest a rare collision between galaxies, potentially illuminating the formation of massive black holes and their role in shaping the universe.
The study found that repeated administration of interferon beta-1b decreased the rate of new 'black hole' lesions but did not affect their duration. This suggests that the drug may be neuroprotective but does not change the underlying pathological process in multiple sclerosis.
Astronomers have found a large population of obscured quasars, which are thought to be hidden behind dust in galaxies. The discovery sheds light on the growth habits of black holes at the heart of active galaxies.
The Millennium Simulation uses sophisticated modeling techniques to recreate evolutionary histories for 20 million galaxies and supermassive black holes. The simulation demonstrates that a few massive black holes can form early enough to account for rare quasars, and provides a new tool for understanding the nature of dark energy.
According to Professor Andrew Hamilton, the core of a black hole is not a singular point of infinite density but rather a hot, dense plasma that siphons matter into itself. This plasma could be the cause of a space traveller's demise in larger black holes.
Recent studies of the cosmic microwave background radiation suggest that small black holes were widespread in the early universe and merged to form larger black holes. This finding could indicate an era in which small black holes were commonplace, with potential telltale evidence in galaxies without a central supermassive black hole.
Researchers have found that some galaxies and their central black holes underwent a phenomenal growth spurt, setting the stage for the birth of quasars. The study used Chandra X-ray observations to track the growth of supermassive black holes alongside the formation of stars in these galaxies.
Astronomers have detected periodic X-ray variations in a galaxy, suggesting a massive black hole with a mass of approximately 10,000 Suns. This finding provides strong evidence for the existence of intermediate-mass black holes, which could bridge the gap between stellar-mass and supermassive black holes.
Researchers have found that black holes in 10 dimensions behave like fluids with near-zero viscosity, which is lower than water. This discovery could revolutionize our understanding of the behavior of matter and energy at extreme temperatures and densities.
Computer simulations of black holes have revealed that the process of matter accretion is more complex than previously thought. The new findings show that magnetic fields play a crucial role in creating violent disturbances in density, velocity, and magnetic field strength near the event horizon.
Researchers used Doppler radar-like technique to track gas around the center of NGC 4395, measuring a mass less than a million solar masses - about 100 times smaller than others of its type. This discovery provides insight into midsize black holes and their role in galaxy formation.
Researchers found that growing black holes release energy that regulates galaxy evolution and black hole growth, matching observed relationships between black hole size and galaxy mass. The simulations also show that smaller galaxies have less gas to form stars, while larger galaxies produce more.
Simulations show that growing black holes release a blast of energy, powering strong winds that prevent material from falling in, inhibiting further growth. This process links black hole mass to the total mass of stars in galaxies, explaining observed phenomena and promising deeper insights into galaxy formation.
The LISA mission will detect low-frequency gravitational waves from the merger of compact objects like stellar-size black holes and neutron stars. By measuring tiny changes in the motion of freely falling test masses, scientists can study these events with unprecedented precision.
Researchers found a high concentration of X-ray sources near the Galactic center, suggesting multiple black holes are present. The presence of these black holes is consistent with the theory that stellar-mass black holes can sink toward the center of the galaxy through dynamical friction.
Astronomers discovered a dense stellar graveyard with thousands of X-ray sources within 70 light years of the Milky Way's center. The discovery supports the idea that dynamical friction could create a massive population of stellar-mass black holes.
Astronomers have discovered that radio jets from black holes can trigger the collapse of interstellar clouds and induce star formation. The jets' collision with dense gas leads to the creation of new stars, bringing 'new life' to these systems.
Scientists have developed a new method to isolate the light from compact regions of black holes using polaroid filters. This allows them to focus on the area surrounding the black hole, revealing new signals such as the 'Balmer edge' feature that provides information about material properties.
A team of astronomers has discovered hundreds of hidden supermassive black holes in the distant universe, invisible to optical telescopes. The new observations combined data from NASA's Hubble Space Telescope, Chandra X-ray Observatory, and Spitzer Space Telescope, revealing objects that were previously thought to be missing.
Astronomers using the European AVO Virtual Observatory have discovered a whole population of obscured, powerful supermassive black holes in the GOODS survey fields. The team found thirty objects, which they believe were underestimated by a factor of two to five.
Physicists at Ohio State University propose a solution to the long-standing information paradox by suggesting that black holes are made up of giant tangles of strings that preserve the information of particles that enter them. This theory resolves the paradox and provides new insights into the nature of black holes.
A team of astronomers has discovered 13 distant quasars, providing valuable insights into the early universe. The most ancient quasars are thought to have formed right along with supermassive black holes, suggesting a rapid transition from the cosmic dark ages to the cosmic renaissance.
By embedding a two-dimensional photonic crystal into the top face of a VCSEL, researchers can accurately design and control the device's mode characteristics. The technology has the potential to push VCSEL performance toward higher power and enable mass-produced devices for high-speed data communication.