Articles tagged with Galaxies
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.