Researchers assessed ATT12's observational capabilities and found it could detect distant galaxies, identify dusty star-forming galaxies, and study galactic gas density. The telescope is planned for construction in Antarctica's dry conditions.
Researchers from McGill and MIT used fast radio bursts and galaxy locations to map the distribution of missing matter, finding it surrounds galaxies and extends four million light-years from them. The discovery supports the idea that black hole jets and other energetic processes fling matter outside galaxies.
A recent study from Florida International University suggests that galaxy mergers are neither necessary nor sufficient to stop galaxies from forming new stars. Instead, slower internal processes are believed to play a much larger role in quenching star formation.
Researchers reveal that missing ordinary matter exists in diffuse clouds surrounding galaxy groups, extending beyond predicted distances. The findings suggest stronger and more violent star activity and black hole jets, pushing matter to larger scales.
Researchers found that galaxies with slowly rotating stellar haloes are more likely to have experienced a major disc flip, where the galaxy's disc changed its orientation by more than 90 degrees. This discovery provides clues about how the Milky Way assembled and may offer indirect hints about the motion of its invisible dark matter halo.
Astronomers at Durham University have discovered the most distant example of a compact, star-forming structure at the heart of a galaxy, dating back over nine billion years. This finding reveals clear evidence of a nuclear disc forming at an early stage in cosmic history.
Researchers have discovered a 'galaxy-killing wind' that could explain the origin of massive dead galaxies in the early universe. Using JWST and ALMA, they imaged a galaxy one billion years after the Big Bang, revealing a huge plume of cold gas extending far away from it.
The study suggests that massive galaxies formed through violent mergers, leading to a rapid burst of star formation and the growth of supermassive black holes. This process prevented these galaxies from producing new stars for over a billion years, leaving them as quiescent galaxies.
Astronomers observed a galaxy protocluster at 1.2 billion years after the Universe's birth, finding it was already shaped by its environment. The Loktak Protocluster had larger, redder galaxies with more rounded shapes than isolated galaxies.
A team of astronomers has produced the most detailed map of the cosmic web, tracing its network of galaxies back to one billion years old. The COSMOS-Web survey, conducted with the largest JWST survey, reveals a more informative large-scale structure than earlier maps.
Astronomers using the James Webb Space Telescope discovered a galaxy that is not rotating, contradicting current theories about galaxy formation. The team believes this galaxy may have been formed after a single collision between two galaxies, making it a rare and unexpected finding.
A new study uses unprecedented simulations to reveal how ultra-faint dwarf galaxies reflect the conditions of the early Universe. These tiny satellite galaxies can provide clues about the properties of dark matter and help test early-Universe physics with upcoming observations.
Ultra-faint dwarf galaxies, tiny satellite galaxies of the Milky Way, can reflect conditions of the early universe, shedding light on galaxy formation and dark matter. Simulations suggest these small galaxies are sensitive to early radiation environment and can probe the universe's earliest climate.
The COLIBRE simulations successfully reproduce real galaxies in the present-day universe and early universe as seen by the James Webb Space Telescope. The models include cold gas and cosmic dust, which strongly affect galaxy appearance in telescopes.
A new study using the Hobby-Eberly Telescope Dark Energy Experiment has discovered over 33,000 hydrogen gas halos surrounding galaxies 10-12 billion years ago. The team's observations have provided a more representative sample for studying the origin and evolution of the first galaxies.
The Small Magellanic Cloud's stars do not orbit around its center due to a direct collision with the Large Magellanic Cloud. The collision disrupted the SMC's internal structure and destroyed its gas rotation, making it a unique case to study galaxy evolution.
Astronomers detect rare cosmic burst from colliding galaxies, which sheds light on how the universe creates heavy elements like gold and platinum. The burst, known as GRB 230906A, is believed to have been triggered by the collision of two neutron stars, releasing a flood of energy and forging heavy elements.
The REGALADE catalogue combines data from 14 widely used catalogues and deep imaging surveys to create a unified place for astronomers to look up galaxy distances and features. This results in precise distance and size measurements for all galaxies, as well as stellar masses for most of them.
Astronomers have used Line Intensity Mapping to create the largest and most accurate 3D map of Lyman alpha emissions in the early universe, adding nuance to the formation of galaxies. The map reveals the location of fainter galaxies and gas, providing insight into the evolution of galaxies and the role of intergalactic gas.
A team of astronomers led by UMass Amherst has discovered a population of dusty, star-forming galaxies at the edge of the universe, formed 13 billion years ago. These galaxies are linked to ultrabright, young galaxies and massive quiescent galaxies, providing new insights into galaxy evolution.
Astronomers from the University of Waterloo have observed a distant jellyfish galaxy, providing rare insight into how galaxies were transformed in the early universe. The discovery challenges previous beliefs about galaxy clusters and their impact on galaxy properties.
Researchers created the highest resolution map of dark matter, showing its interaction with normal matter through gravity. The new data from NASA's James Webb Space Telescope confirms previous research and provides new details about dark matter's influence on the Universe.
A recent study suggests that dark stars could provide solutions to three pressing puzzles of the high-redshift universe: blue monster galaxies, overmassive black hole galaxies, and little red dots. Dark stars form in dark matter-rich environments and can grow to become supermassive, complementing standard models of galaxy formation.
Researchers identified nine objects with characteristics of stars and galaxies, sparking new questions about the cosmos. These 'platypus galaxies' have narrow emission lines indicative of active star formation, defying expectations.
Scientists at CU Boulder have solved a pressing mystery about the universe's gravitational wave background by revealing the role of smaller galaxies in galaxy evolution. The new study suggests that when a smaller supermassive black hole merges with a larger one, the smaller black hole gains mass, producing larger gravitational waves.
Researchers reconstruct Milky Way's evolution from its earliest phases to present day, revealing a tumultuous youth and chaotic conditions. The study provides new insights into galaxy formation and growth, highlighting the need for refinement in theoretical predictions.
Scientists have found that active galactic nuclei are two to six times more common in merging galaxies than non-merging counterparts. Galaxy mergers were most strongly associated with bright, dust-cloaked supermassive black holes linked to rapid growth.
A new study using advanced computer simulations has shed light on the mysterious chemical history of the Milky Way. Researchers found that galaxies like the Milky Way can develop two distinct chemical sequences through various mechanisms, challenging previous assumptions about the role of cosmic gas flows and galaxy mergers.
Researchers have identified a massive cosmic filament containing 280 galaxies, many of which are spinning in the same direction as the filament itself. The discovery provides rare insight into how galaxies gain their spin and could inform future efforts to model intrinsic alignments of galaxies.
A team of astronomers from ICRAR has released new data showing that a galaxy's 'neighbourhood' plays a major role in its evolution over time. The study found that where a galaxy lives strongly influences its shape, size and growth rate in the distant Universe.
A study from Bielefeld University reveals that the solar system is moving more than three times faster than predicted by current models. This deviation was detected using data from radio galaxies, which emit strong radio waves and can penetrate dust and gas.
Researchers used the James Webb Space Telescope to study young galaxies in the early universe, finding most were turbulent and 'clumpy'. Despite this chaos, galaxy dynamics show a gradual transition towards ordered structures, suggesting that galaxies like our Milky Way formed through frequent mergers and bursts of star formation.
Researchers used the James Webb Space Telescope to study 12 quasars from 12.9 billion years ago, revealing mature galaxies with active supermassive black holes. This challenges previous research suggesting black hole activity suppresses galaxy growth, instead showing a complex relationship between the two.
Researchers at Rutgers University uncovered evidence of how galaxies expand by tracing the invisible scaffolding of the universe created by dark matter. They analyzed large samples of special galaxies called Lyman-alpha emitters to study galaxy formation and evolution over billions of years.
Astronomers suggest that tiny red objects spotted by NASA's James Webb Space Telescope could be giant spheres of hot gas powered by supermassive black holes. The objects, called 'universe breakers,' defy prior understanding of galaxy formation and may represent an entirely new class of celestial object.
Researchers used infrared images to spot bright objects, then applied the 'dropout' technique to confirm their nature. The study could challenge current ideas about galaxy formation in the early universe if confirmed.
Researchers studied similar spiral galaxies and found they 'dance' with closely located dwarf satellites, potentially revealing the formation and evolution of our galaxy's satellite system. The study aims to refine models of galaxy evolution and cosmic structure, offering new insights into our understanding of the universe.
A new study by Dartmouth astronomers has mapped 355 candidate satellite galaxies around dwarf galaxies, tripling the number previously surveyed. The researchers aim to understand how external conditions influence satellite formation and uncover insights into dark matter's nature.
Researchers used the Dark Energy Camera to image a 'bridge' of diffuse light spanning roughly a million light years between two galaxies in Abell 3667. The findings suggest that the brightest galaxies in the cluster are actively merging, with one larger galaxy stealing stars from a smaller one.
Researchers have discovered star-shredding black holes in dusty galaxies, confirming that these events are powered by dormant black hole accretion. The study uses the James Webb Space Telescope to detect clear fingerprints of black hole activity in four galaxies, revealing key differences between active and dormant black holes.
New research predicts the existence of 80-100 additional satellite galaxies surrounding the Milky Way, orbiting at close distances. These 'orphan' galaxies are lost in most simulations but should have survived in the real Universe.
Researchers discovered high-velocity clouds in the nearby spiral galaxy M83, which moved at speeds significantly different from the galaxy's overall speed of rotation. The findings suggest that these clouds originated outside the galaxy, providing new insights into how galaxies acquire fresh gas and sustain star formation over billions...
Astronomers have identified thin and thick disks in distant galaxies using JWST images, revealing a consistent trend of sequential disk formation. The study estimates the thin disk formation time for Milky Way-sized galaxies to be around 8 billion years ago.
Researchers surveyed luminous infrared galaxies to gain insight into galaxy formation in the early universe and possibly the Milky Way. They discovered massive clumps of newborn stars, unlike anything seen in the Milky Way.
Astronomers have identified dozens of small galaxies that played a key role in transforming the early universe into the one we know today. These tiny but mighty galaxies produced ultraviolet light, which drove the reionization of the universe.
The COSMOS-Web field maps nearly 800,000 galaxies spanning 98% of cosmic time, challenging existing notions of the infant universe. Researchers see roughly 10 times more galaxies than expected at incredible distances, sparking new questions about the early universe and its mysteries.
Researchers have found that most Lyman Alpha Emitters (LAEs) are experiencing their first major burst of star formation, revealing crucial insights into galaxy development and the early stages of the universe. The study sheds light on the Milky Way's origin story, providing key information about how galaxies grow and evolve.
A newly discovered cluster of eleven quasars has shattered the previous record, with the Cosmic Himalayas forming a boundary between galaxy groups. This structure forces astronomers to rethink quasar formation scenarios, leading to new theories and potential insights into the evolution of the Universe.
A newly discovered cluster of eleven quasars has shattered the previous record of five, with the Cosmic Himalayas quasar cluster sitting on the boundary between two groups of galaxies. This structure cannot be explained by conventional theories and forces astronomers to rethink formation scenarios for quasars.
Scientists used NASA's Hubble and Gaia space telescopes to simulate the evolution of the Milky Way and Andromeda over 10 billion years. Contrary to previous beliefs, they found a only 2% probability of collision within five billion years.
Researchers use ALMA to observe J0107a, a 'monster' galaxy 11.1 billion years ago. They find similarities with modern galaxies in gas distribution and motion, but higher concentrations and faster gas flow rates.
A new study of diffuse dwarf galaxies has revealed an exceptionally strong clustering pattern, contradicting the established understanding of galaxy clustering. The researchers propose a new model of dark matter based on the Self-Interacting Dark Matter (SIDM) theory.
Researchers at ICRAR have found that galaxies forming stars rely on the location of atomic hydrogen gas, not its total amount. Higher-resolution observations allowed for unprecedented mapping of gas distribution in 1,000 galaxies.
Researchers have detected 1,678 galaxy groups or proto-clusters with unprecedented insights into the formation and evolution of galaxies. The study provides a unique view of how galaxies have evolved since the universe was under a billion years old.
A team of researchers at Nagoya University has discovered a fast-moving, high-temperature gas flow in the center of the Centaurus cluster of galaxies. This finding may solve the 'cooling flow problem', which explains why galaxy clusters appear to be warm despite emitting X-rays.
Astronomers have discovered a massive spiral galaxy resembling the Milky Way, formed just 1 billion years after the Big Bang. The galaxy, Zhúlóng, exhibits a mature structure with a central old bulge and large star-forming disk, challenging our understanding of galaxy formation.
Researchers have found evidence of a new population of faint galaxies hidden in the far-infrared sky, which could break current models of galaxy numbers and evolution. The discovery was made using data from the Herschel Space Observatory, which revealed a deeper image of the universe than ever before.
A new study proposes a third category of galaxies: red star-forming. These galaxies produce low-mass stars and may have played a significant role in the universe's history. The findings could change our understanding of galaxy evolution, star formation, and the life cycle of galaxies.
A new study by the University of Oulu has directly observed the merger of star clusters in dwarf galaxies for the first time, shedding light on their formation. The observations confirm that compact star clusters form through the cannibalization of smaller globular clusters at the centers of these galaxies.