Articles tagged with Galaxies
Researchers found that intense ultraviolet light acted like a 'cosmic leaf blower', pushing gas and dust away from stars in the early universe, making their galaxies appear brighter. This effect likely contributes to the brightness of early galaxies by clearing the line of sight between stars.
Researchers have discovered magnetic reconnection eruptions and Coronal Mass Ejections near supermassive black holes, similar to solar storms. The 'Neupert effect' was observed in the galaxy NGC 3783, indicating the same physical processes underlying solar storms occur in black hole environments.
Researchers at Eötvös Loránd University found statistical evidence that some supermassive black holes are ejected from their galaxy centers after forming. Quasars containing faster-moving black holes are, on average, redder, indicating more dust obscures them.
Researchers found that white dwarf stars can exhibit a range of colors, including green, pink, and purple, due to the density of their atmospheres. The study used data from existing spectra to calculate the color each star's light would appear as to the human eye, revealing new insights into the color spectrum of these stellar remnants.
Researchers found that early galaxies were already producing and dispersing heavy elements, such as oxygen and carbon, 500 million years after the Big Bang. This discovery challenges previous assumptions and provides insights into the early universe's chemical evolution.
A new survey of 29 massive stars in extremely metal-poor galaxies reveals unexpectedly weak stellar winds, delivering the largest-ever dataset of its kind. The findings could reshape our understanding of how galaxies formed in the early universe, and provide insights into the evolution of massive stars.
The FAST All Sky HI Survey has detected 156,411 extragalactic HI sources, nearly four times the previous record, and achieved a median sensitivity of 0.57 mJy/beam. The survey provides a high-quality dataset for galaxy evolution studies in the SKA era.
Astronomers have discovered the most distant progenitor to a galaxy supercluster, supporting existing theories of how galaxy clusters evolve. The study used data from the ODIN survey to map the 3D distribution of galaxies in the COSMOS-z3.1-A and COSMOS-z3.1-C clusters.
Astronomers have discovered a new population of faint, rapidly fading remnant radio galaxies, revealing a shorter, more dynamic afterlife of black hole jets. The study found that these remnants are relatively young, with ages ranging from 8-42 million years, and span a wide range of evolutionary stages.
Researchers have discovered a globular cluster stellar stream in another galaxy, offering new insights into the nature of dark matter. The study demonstrates that these streams can be used to measure dark matter content beyond our own galaxy, opening doors to a broader understanding of its behavior.
Astronomers have discovered the first globular cluster stellar stream outside the Milky Way, providing a powerful tool for studying dark matter. The study uses the stream's shape to reconstruct the galaxy's gravitational field and infer how dark matter shaped the stars' orbits.
Researchers from the University of Missouri discovered that the ratio of large and small stars in distant galaxies depends on their environment, potentially altering how scientists estimate galaxy mass and age. This breakthrough could lead to more accurate estimates and a better understanding of the universe's history.
The Local Volume Mapper is capturing light to reveal the physics and chemistry of stellar birthplaces across vast expanses of the sky in unprecedented detail. Astronomers are analyzing specific spectral lines to map the precise temperature, density, chemical abundance, and motion of interstellar gas.
The SDSS-V survey has released its twentieth public data release (DR20), providing a massive catalog of high-quality spectra of stars across the Milky Way. The dataset includes over two million total spectra, revealing temperatures, ages, and chemical compositions of stars.
The study provides the largest, most uniform spectroscopic follow-up of X-ray sources ever assembled, capturing tens of thousands of X-ray-emitting galaxy clusters. It reveals that rapidly growing giant black holes were surprisingly common in the early Universe and more 'hidden' black holes have been uncovered.
The Sloan Digital Sky Survey has released its 20th data set, featuring over three million spectra of stars and galaxies, as well as 18 new value-added catalogs. This release marks a significant expansion of the survey's efforts, integrating full all-sky panoptic spectroscopy across both hemispheres.
A team of researchers has discovered that supermassive black hole winds are 100 times more powerful than previously thought, carrying energy across 300,000 light-year distances. This finding demonstrates the explosive winds' impact on space beyond galaxies.
Researchers used machine learning to identify seven rare quasar candidates from a list of 800,000 quasars. The discovery offers an opportunity to expand knowledge of how quasars and their host galaxies work, as well as understanding our own galaxy's evolution.
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.
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 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.
The European Space Agency's Euclid space telescope has discovered 31 of the oldest quasars ever found, revealing insights into the universe's first 670 million years. The two most ancient quasars have redshifts of 7.77 and 7.69, setting a new record for their age.
A team of scientists has discovered a new neutrino source candidate, an extremely bright galaxy called Shadow Blaster, located about 11 billion light-years away. The galaxy's location and brightness made it a promising candidate for the source of high-energy neutrinos.
Astronomers have detected the [O I] 145 µm emission line in four typical star-forming galaxies, which serves as a clear tracer of neutral gas. This detection provides unprecedented detail on the physical and chemical conditions of star-forming material in these distant galaxies.
New study by University of Southampton confirms the universe's expansion is still accelerating as previously found, debunking 2025 claims that the cosmos was slowing. The team re-evaluated data using Type Ia supernovae to calculate vast cosmic distances and found no error in their methods.
A team of astronomers used JWST to detect the motion of stars near a galaxy's center affected by a dormant black hole's gravity. The findings suggest that densest galaxies were sites of rapid black hole growth early in cosmic history.
Researchers at Kyushu University used 3D computer simulations to understand the physics behind hub-and-spoke patterns in star-forming regions. The study shows that oblique shocks create invisible channels guiding compressed gas into central filaments, forming the radial shape of baby stars' cradles.
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.
A team at the University of Arizona discovered exceptionally fast and powerful galactic winds from quasars a billion years after the Big Bang. These winds could have caused galaxies to lose gas supplies, effectively shutting down star formation. The study suggests that quasars with extreme outflows were more common in the early univers...
The study reveals that more massive young star clusters clear away their natal gas faster than lower-mass clusters. This has implications for our understanding of star formation and how the young stars affect their surroundings.
An international team of astronomers, led by Daniela Calzetti, has observed the 'natal clouds' surrounding young star clusters for the first time. The study reveals that massive star clusters disperse their gaseous shroud faster and light up their galaxy earlier than smaller ones.
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.
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.
A study led by University of California, Riverside graduate student Yash Aggarwal suggests that dark matter decays could have seeded the direct collapse of galaxies into giant black holes. The research found that a window of dark matter masses between 24 and 27 electronvolts could produce conditions for black hole formation.
A study suggests that self-interacting dark matter (SIDM) can explain unusual gravitational effects observed in various astrophysical environments. Dense clumps of SIDM can account for high-density structures in the universe, providing a promising candidate for explaining small-scale cosmic structure.
Researchers suggest that dark matter may consist of multiple particles, whose behavior varies depending on the cosmic environment. This could explain why a signal observed at the center of our galaxy is not seen in dwarf galaxies.
Researchers from Kyushu University used ALMA to observe a baby star producing a giant ring of gas about 1,000 au in size, which helps the star release excess energy. The team found that this ring is slightly warmer than its surroundings and hypothesize it's produced through magnetic field threading.
Astronomers have captured unprecedented detail of cosmic gas in the Milky Way's Central Molecular Zone, revealing intricate chemistry and complex star-forming processes. The dataset provides a unique view of the raw material from which stars form, shedding light on galaxy evolution and the birth of massive stars.
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.
A study using the James Webb Space Telescope found that supermassive black holes can suppress star growth not only in their host galaxy but also in neighboring galaxies within a million-light-year radius. This discovery reveals a larger impact of quasars on galaxy evolution, contradicting previous assumptions.
Researchers from the University of Copenhagen have explained the mysterious 'red dots' seen in James Webb Space Telescope images as young black holes. The discovery provides insight into how the universe's first black holes were born and sheds light on their early development.
Astronomers have spotted an ancient galaxy that was slowly starved of fuel by a supermassive black hole. The galaxy's lack of cold gas prevented it from forming new stars, despite its relatively young age. Repeated episodes of heating and gas removal by the black hole likely drained the galaxy's fuel in as little as 16-220 million years.
A team of researchers has observed a massive galaxy cluster that challenges existing models of the universe's evolution. The cluster's unusual structure and high density of cold, neutral hydrogen gas suggest a different history than previously thought. This discovery raises questions about the fate of large structures in the universe.
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 have found a galaxy cluster with scorching hot gas just 1.4 billion years after the Big Bang, five times hotter than predicted, and containing three supermassive black holes that pumped energy into the surroundings. This discovery could upend current models of galaxy cluster formation and evolution.
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.
Astronomers discover galaxy Virgil with dual personality – ordinary in visible light but harboring massive black hole. JWST observations reveal hidden nature of Virgil, challenging current models of black hole formation.
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.
Astronomers have observed a record-breaking gamma-ray burst that lasted nearly seven hours, challenging existing models for these events. The burst's unusual duration and properties suggest multiple possible causes, including the collapse of a massive star or the collision of exotic stellar remnants.
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.
Researchers at RIKEN successfully simulated the Milky Way Galaxy with over 100 billion individual stars, far surpassing previous state-of-the-art models. This achievement demonstrates the power of AI-accelerated simulations in tackling complex multi-scale problems in astrophysics and beyond.
Astronomers detect a distant galaxy with temperatures of 90 Kelvin, indicating an extreme star factory that could have produced stars at a rate 180 times faster than the Milky Way. This discovery provides insight into how galaxies formed quickly in the early universe.
A team from the International Centre for Radio Astronomy Research has assembled a record-breaking radio colour image of the Milky Way. The unprecedented level of detail offers new insights into the galaxy's radio emission and structure.
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.
Astronomers detected complex organic molecules in ices outside the Milky Way for the first time, finding five different carbon-based compounds, including methanol and acetic acid. This discovery sheds light on how chemical ingredients for life spread throughout the cosmos.
A mysterious glow in the Milky Way could be a clue to dark matter's existence. Researchers used supercomputers to simulate dark matter locations and found matches with actual gamma ray maps.
Researchers at Goethe University Frankfurt used complex simulations to study the origin of powerful jets emitted by black holes. They discovered that magnetic reconnection is involved in extracting rotational energy and powering these jets.