Articles tagged with Galaxies
Researchers found that the 'caustic curve' shape, seen in sunlight reflections on water or boat hulls, is connected to gravitational lensing effects in distant galaxies. The discovery could enable scientists to map dark matter clumps using caustic violations.
UK astronomers using NASA Swift Satellite captured an ultraviolet spectrum of a gamma ray burst just 251 seconds after its onset, marking the earliest ever recorded. This breakthrough allows for calculations of distance and brightness within hundreds of seconds and provides new insights into GRB causes and host galaxies.
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.
Researchers at Durham University's Institute for Computational Cosmology created simulations to predict galaxy formation and dark matter effects. The work aims to improve understanding of dark matter, a mysterious substance making up 80% of the Universe's mass.
Astronomers have identified gas molecules in the host galaxy of a gamma-ray burst, providing insight into star formation when the universe was about one-sixth its present age. The study found hydrogen and carbon monoxide absorption lines, suggesting a thick molecular cloud similar to those that spawn stars in our galaxy today.
Researchers used data from NASA's Chandra X-ray Observatory and Compton Gamma Ray Observatory to study the Bullet Cluster, where two large clusters of galaxies collided. The results show that the antimatter fraction in the cluster is less than three parts per million, ruling out significant amounts of antimatter on scales of about 65 m...
Researchers identified an unexpected motion in distant galaxy clusters, suggesting gravitational attraction beyond the observable universe. The 'dark flow' is constant out to a billion light-years and flies in the face of predictions from standard cosmological models.
Astronomers study massive galaxies in clusters to understand their growth. The team observed four galaxy groups and found that three of them have a bright companion galaxy, indicating merging systems.
The James Webb Space Telescope sunshield, crucial to the mission's success, has completed its preliminary design review. The five-layer sunshield will deploy in space to shade the telescope optics and enable it to reach proper operating temperature.
Astronomers have measured the distribution and motions of thousands of galaxies in the distant Universe using ESO's VLT. This study provides a powerful way to tackle the mystery of dark energy, with results supporting the simplest form of dark energy.
For the first time, astronomers have directly visualized the distribution of dark matter in a supercluster, allowing for the detection of irregular clumps and detailed shapes. This breakthrough study, led by UBC researcher Catherine Heymans, uses NASA's Hubble Space Telescope to map the Abell 901/902 supercluster.
A new study using Chandra X-ray Observatory results provides evidence that many supermassive black holes are spinning extremely rapidly. The research suggests that these fast-spinning black holes can drive powerful jets, pumping energy into their environment and affecting galaxy growth.
Astronomers have discovered a rare type of star system containing a black hole that suddenly began glowing brightly with X-rays. The system, dubbed CXOU J132518.2-430304, is thought to be a binary star system where one star collapsed to form a black hole.
Astronomers have detected a mysterious type of cosmic explosion, known as a short gamma-ray burst (GRB), 7.4 billion years ago, more than halfway back to the Big Bang. This discovery dramatically moves back the time at which we know short GRBs were exploding.
Astronomers have detected a record-breaking short gamma-ray burst (GRB) 7.4 billion years ago, revealing new insights into their formation mechanisms.
A team of astronomers discovered a long-duration gamma-ray burst (GRB) in the middle of nowhere, thousands of light-years from the nearest galaxy. The GRB's afterglow was bright and fast-fading, but there was no dense gas or dust to absorb its light.
Astronomers analyze galaxy clusters and discover that dark matter, a mysterious invisible force, has an incredibly long lifetime. The research suggests that axions, a type of particle with extra dimensions, could be the culprit behind this prolonged existence.
Astronomers discover a bright arc of extremely hot gas in a massive galaxy cluster, suggesting an exceptionally dramatic event, such as a collision between two clusters. The temperature and mass of the cluster make it a giant among giants, with a quadrillion suns' worth of mass bound by its hot gas.
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.
A team of astronomers has discovered a unique structure of dark matter in the galaxy cluster Cl 0024+17, with a ring shape unlike that of galaxies and hot gas. The discovery is among the strongest evidence for dark matter's existence, supporting theoretical models of its behavior under gravity.
Researchers used COSMOS field data to measure large-scale distribution of matter, revealing concentration of luminous and dark matter. The 3D map provides insight into the formation and evolution of galaxies and may shed light on dark energy.
The microshutters will enable scientists to block unwanted light from objects closer to the camera in space, letting the light from faraway objects shine through. This technology allows the telescope to focus on the faint light of stars and galaxies so far away, they formed early in the history of the universe.
Astronomers have created the first 3D map of the universe's dark matter distribution, revealing a web-like structure that confirms conventional theories on how galaxies formed. The map was derived from the Cosmic Evolution Survey and offers unprecedented detail on the large-scale filamentary structure of dark matter.
George Smoot's discovery of miniscule temperature variations in the infant universe revealed a pattern consistent with the Big Bang theory. This finding, supported by subsequent experiments, confirmed the cosmos' origins and provided evidence for gravity's role in shaping the universe's structure.
A new study reveals the existence of more than one type of Type Ia supernova, with SNLS-03D3bb being over twice as bright and half as massive as typical examples. This finding opens up new possibilities for understanding these cosmic events.
A team of scientists at the University of Chicago has verified the main features of the cold dark matter model by comparing supercomputer simulations to recent astronomical observations. The simulations accurately reproduced the distribution of galaxies in the early stages of the universe's evolution.
Researchers have created a massive 3-D map of the universe, mapping the distribution of galaxies and providing new insights into dark energy. The map uses luminous red galaxies as 'lighthouses' to measure distances, covering vast scales of up to a billion light-years across.
Astronomers have created detailed maps of invisible dark matter in two young galaxy clusters, lending credence to the theory that galaxies form at dense regions of cosmic webs. The study used the Hubble Space Telescope's Advanced Camera for Surveys to overcome atmospheric turbulence and measure subtle gravitational lensing effects.
Scientists have discovered energetic plumes extending 300,000 light years into a massive galaxy cluster. The plumes are caused by explosive venting from a supermassive black hole and demonstrate the far-reaching influence of a black hole on intergalactic distances.
The HETE-2 satellite has solved the mystery of short gamma-ray bursts, revealing colliding compact stars as their likely cause. The discovery provides significant findings, including first observations of optical afterglows and secure measurements of distance to a short burst.
A team of astronomers has discovered a large population of galaxies formed between 9 and 12 billion years ago, contradicting previous estimates that the Universe had not yet formed many stars in the first billion years. The findings suggest that stars formed two to three times faster than previously thought.
Case Western Reserve University astronomers have captured a deep, wide-field image of the Virgo Cluster, revealing a complex web of intracluster starlight. The faint starlight is made up of stars ripped out of galaxies as they collide, providing an 'archaeological record' of violent cluster galaxy lives.
A Penn-led team has launched a balloon-borne telescope, BLAST, to survey the universe for faint stellar objects and gain insights into the formation of stars and galaxies. The telescope will capture light at three wavelengths, allowing astronomers to determine an object's distance and luminosity.
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 captured ancient, 9-billion-year-old light from a massive galaxy cluster, providing a snapshot of the universe at 5 billion years old. The discovery confirms that galaxy clusters formed in a way consistent with recent structures.
Researchers are exploring alternative explanations for dark energy, including the possibility of modified gravity laws and a multiverse. String theory suggests that the value of the cosmological constant may be very small, while another speaker proposes using
University of Pennsylvania astrophysicist Licia Verde outlines a multi-disciplinary approach to studying dark energy. The investigation draws on data from galaxy surveys, supernovae, and the Cosmic Microwave Background, providing clues about this enigmatic component.
Researchers found that strong stellar winds around young red dwarfs may be responsible for removing dust and debris disks. The discovery provides a potential explanation for the rare occurrence of debris disks among red dwarfs, but further observations are needed to confirm this hypothesis.
A team of researchers uses the Keck laser system to observe distant galaxies in unprecedented detail, finding that some systems exhibit old stars despite recent mergers. This discovery challenges prevailing theories of galaxy formation and may help explain the existence of large galaxies with little young star population.
A Yale astronomer and her colleagues used gravitational lensing techniques to create a spatial map demonstrating the clumped substructure of dark matter inside galaxy clusters. The study found an excellent agreement between observations and theoretical predictions, supporting the concordance model.
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.
The Gemini Observatory has released a breathtaking image of Stephan's Quintet, capturing the intricate interactions between five galaxies. The image showcases sweeping arches of gas and dust, tracing the ongoing dance of gravitational forces that have warped their structures over millions of years.
A recent study has revealed surprisingly mature galaxies in the early universe, contradicting the long-held hierarchical model of galaxy formation. The Gemini Deep Deep Survey found that a large fraction of stars in massive galaxies were already present at 8 billion years old.
A new theory by Jason Tumlinson and colleagues reconciles two conflicting pieces of evidence on the nature of the first stars. The theory suggests that these early stars were smaller than previously thought, with masses between 20-100 times that of the sun.
The CDMS II experiment has narrowed the search for WIMPs, a type of dark matter particle. The results show that the interaction rate of a WIMP with ordinary matter should be less than one interaction every 25 days per kilogram of germanium.
Researchers from Cardiff University suggest that a large comet impact could throw material containing micro-organisms out of the planet's atmosphere, infecting hundreds of millions of nascent planetary systems. This viable bacterial outflow would survive heat and radiation, ultimately spreading Earth-life across the galaxy.
Astronomers have discovered two unique rings of dust illuminated by the afterglow of a gamma-ray burst in our galaxy. The rings, caused by dust scattering X-rays from the burst, reveal new insights into the distribution and behavior of dust in the Galaxy.
The Gemini Deep Deep Survey has revealed a greater abundance of more massive and older galaxies than expected, dating back to the early universe. The discovery challenges current models of galaxy formation and suggests an accelerated growth phase for galaxies.
The STELLAR and MERCURY I studies show CRESTOR significantly improves key apolipoprotein and lipid ratios, including Apo B, Apo A-I, and the Apo B:Apo A-I ratio, in patients with hypercholesterolaemia. These findings support CRESTOR's benefits in reducing cardiovascular disease risk.
The team reconstructed a mass map of the galaxy cluster using NASA/ESA Hubble Space Telescope data, tracing dark matter's distribution with respect to galaxies. The study reveals that dark matter clumps together in certain regions, supporting the idea that clusters assemble through the merger of smaller groups.
A study published by the Mayo Clinic found that 55% of golfers with the 'yips' described physical symptoms, while only 22% attributed them to psychology. The research suggests a continuum of causes for the condition, including performance anxiety and focal dystonia.
Scientists have developed a new theory explaining the formation of large-scale magnetic fields in galaxies, which twist and expand like elastic ribbons. The theory resolves a long-standing problem in astrophysics by showing how turbulence creates opposing small-scale fields that eventually suppress growth.
Researchers using galaxy cluster surveys can measure the equation of state of dark energy, which would provide clues about its nature and origin. By studying scaling relations and X-ray emission, scientists hope to determine the essence of dark energy.
The DEIMOS instrument will multiply the power of current Keck spectroscopy by a factor of seven, enabling observations of distant galaxies and shedding light on the formation and evolution of galaxies. With its massive detector and advanced optics, DEIMOS will create the most comprehensive map of the distant universe ever attempted.
Astronomers have shed new light on dark matter distribution by tracing it closely to galaxy patterns. They found that dark matter is distributed in a parallel pattern to galaxies and makes up about seven times more mass than ordinary matter.
The Interplanetary Network detected a gigantic gamma-ray burst, the most distant ever observed, from a dying star 30 times more massive than the sun. The burst is believed to have occurred 11 billion years ago and has been traveling through space for the same amount of time.
Astronomer Alberto Conti and colleagues have developed a new technique to analyze massive galaxy data using computer analysis. By combining theoretical analysis with statistical techniques, they aim to uncover the most important attributes of galaxies that can be observed.
Despite intensive searches, only a few gamma ray burst counterparts have been found, leaving scientists with more questions than answers. The lack of consistent patterns hampers the search, but continued observations with powerful instruments may help clarify the issue.
The Hobby-Eberly Telescope has taken its first look at the universe, demonstrating its novel design and paving the way for groundbreaking astronomical discoveries. The telescope's innovative design eliminates expensive features while tracking objects with precision, allowing for efficient and cost-effective large-scale observations.