Astronomers have discovered a giant galaxy surrounding the most distant black hole ever found, 12.8 billion light-years from Earth. The galaxy is as large as the Milky Way and harbors a supermassive black hole with at least a billion times more matter than our sun.
SourceUniversity of Hawaii at Manoa·JournalMonthly Notices of the Royal Astronomical Society·DateSep 2, 2009
Researchers found that galaxy collisions 'puff up' a galactic disk, producing stellar rings and flared edges. The Milky Way's puffy appearance is likely due to interactions with satellite galaxies and dark matter.
Katherine Rhode's five-year NSF CAREER award will fund a wide-field imaging survey of globular cluster systems in giant galaxies up to 65 million light years away. The goal is to quantify properties and test theories on galaxy formation.
Researchers measured the motion of stars in a distant galaxy and found they are moving at incredible speeds, contradicting expectations of small galaxy size.
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Astronomers discover rare 'Green Pea' galaxies through Galaxy Zoo project, finding compact galaxies forming stars at high rates. The galaxies, 10 times smaller than Milky Way and 100 times less massive, are surprisingly active in star formation.
SourceYale University·JournalMonthly Notices of the Royal Astronomical Society·DateJul 27, 2009
The NASA Fermi Gamma-ray Space Telescope has discovered a third class of active galaxies that emit gamma rays, opening a new window in the field. The telescope has detected gamma rays from dozens of galaxies beyond our own, including Seyfert galaxies and blazars.
A team of researchers led by UC Riverside astronomer Gillian Wilson has completed the largest ever survey of very distant galaxy clusters. The SpARCS survey detects galaxy clusters using deep optical observations and infrared data from the Spitzer Space Telescope, revealing about 200 new cluster candidates.
A team of astronomers has directly measured the distance to a galaxy, providing a precise tool for unraveling the mystery of Dark Energy. The technique uses water molecules in disks orbiting central black holes to amplify radio waves, enabling measurements up to 160 million light-years away.
SourceNational Radio Astronomy Observatory·DateJun 8, 2009
A rare radio supernova has been detected in the nearby galaxy M82, providing valuable opportunities for studying star formation and supernovas. The discovery was made using the Allen Telescope Array, which will also search for intelligent life signals around other stars.
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Using XMM-Newton's new data, astronomers have mapped the region around a supermassive black hole, estimating its mass at 3-5 million solar masses. The observations also reveal rapid spinning and accretion rates that verge on theoretical limits.
New calculations suggest hundreds of massive rogue black holes are left over from the early universe, potentially wandering the Milky Way's outer reaches. These relics could provide clues about galaxy formation history and the formation of black holes in the early universe.
SourceCenter for Astrophysics | Harvard & Smithsonian·JournalMonthly Notices of the Royal Astronomical Society·DateApr 29, 2009
A deep Chandra X-ray image has resolved a long-standing mystery about an X-ray glow along the plane of the Galaxy. The image reveals hundreds of point-like X-ray sources causing the glow, implying millions of such sources are responsible.
Astronomers have identified a triple merger of four separate galaxy clusters, the first time such a phenomenon has been documented. The galaxy clusters are involved in a cosmic free-for-all, with one collision after another occurring as galaxies pour into a region already full of galaxies.
SourceChandra X-ray Center·JournalThe Astrophysical Journal Letters·DateApr 16, 2009
A team of astronomers has found a sample of massive galaxies with properties suggesting they may have formed recently, running counter to widely-held beliefs. The discovery challenges our understanding of galaxy formation and evolution, offering new opportunities for research into the origin and early history of galaxies.
SourceIndiana University·JournalThe Astrophysical Journal Letters·DateApr 10, 2009
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An international team of astrophysicists used simultaneous observations from optical, X-ray, and gamma-ray telescopes to uncover complex changes in PKS 2155-304's radiation. The findings challenge current theories on how radiation is generated in blazars.
Astronomers have discovered star birth within a cloud of primordial gas, known as the Leo Ring, which lacks dark matter and heavy elements. This finding suggests that new galaxies may have formed through a distinct process, potentially providing insight into the early Universe.
SourceCarnegie Institution for Science·JournalNature·DateFeb 18, 2009
Astronomers have identified a new type of dwarf galaxy, formed out of pristine gas without dark matter. Led by Johns Hopkins University, the discovery was made using the Galaxy Evolution Explorer and suggests that these galaxies may be common throughout the early universe.
SourceJohns Hopkins University·JournalNature·DateFeb 18, 2009
Astronomers are studying a mysterious gamma-ray emission from the center of the Milky Way galaxy, which is surprising given the presence of massive stars and black holes. The emission is thought to be caused by exotic particles such as dark matter or the decay of radioactive elements.
In a groundbreaking study, scientists have discovered that stars were forming at an incredible rate in the core region of an infant galaxy. With a diameter of just 4000 light-years, the star-forming core of J1148+5251 is incredibly productive and reaches its physical limit.
SourceMax-Planck-Gesellschaft·JournalNature·DateFeb 5, 2009
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A Cornell-led team has observed dust forming around a dying star in a nearby galaxy, providing insights into the early universe and the evolution of galaxies. The discovery sheds new light on how cosmic dust was created in the universe's early stages.
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.
The Milky Way galaxy is rotating about 100,000 miles per hour faster than previously understood, increasing its mass by 50 percent. This increase in speed and mass brings the Milky Way closer to colliding with the Andromeda Galaxy or smaller nearby galaxies.
SourceNational Radio Astronomy Observatory·DateJan 5, 2009
The University of Virginia is conducting a new project, APOGEE, as part of the Sloan Digital Sky Survey III to study the chemical and dynamical fingerprints of Milky Way red giant stars. The team aims to understand the assembly of the Milky Way galaxy and its evolution.
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Researchers discovered glycolaldehyde, a basic sugar molecule, towards a star-forming region where habitable planets may exist. The detection suggests that the production of this key ingredient for life could be common throughout the galaxy.
SourceScience and Technology Facilities Council·JournalThe Astrophysical Journal Letters·DateNov 25, 2008
Researchers used a massive computer simulation to 'see' gamma-rays given off by dark matter in the Milky Way galaxy. They predict that these gamma-rays should glow in a characteristic pattern near the Sun, which could help detect invisible clumps of dark matter.
A team of scientists used a natural cosmic lens to capture an image of a distant galaxy in the early Universe. The image shows a massive reservoir of gas and a supermassive black hole feeding a burst of star formation, indicating that the galaxy has collided with another.
A team of scientists has discovered a new population of colliding galaxy clusters that were previously undetected at shorter wavelengths. The discovery confirms theoretical predictions about particle acceleration through turbulent waves generated by violent collisions.
SourceNaval Research Laboratory·JournalNature·DateOct 15, 2008
Astronomers used gravitational lensing and adaptive optics to observe a young star-forming galaxy, finding clear signs of orderly rotation and evidence for a spiral disk with a central nucleus. The study demonstrates the power of future telescopes like the Thirty Meter Telescope.
SourceCalifornia Institute of Technology·JournalNature·DateOct 8, 2008
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Researchers at Durham University and Caltech used gravitational lensing to study a young star-forming galaxy in the distant Universe, revealing its internal velocity structure and spiral disk. The findings provide insight into how the galaxy evolved into a present-day system like our Milky Way.
Astronomers have discovered evidence that high-speed collisions between large elliptical galaxies can prevent new stars from forming. The study found that gravitational interactions can heat up gas, making it difficult for stars to cool and form.
SourceYale University·JournalThe Astrophysical Journal Letters·DateOct 7, 2008
Researchers have directly measured a nascent galaxy's magnetic field, finding it is at least 10 times stronger than the average value in the Milky Way. This unexpected result presents a challenge to the leading theory of magnetic field generation and suggests that magnetic fields may play a key role in the evolution of galaxies.
SourceUniversity of California - San Diego·JournalNature·DateOct 1, 2008
New simulations suggest that stars like our sun can migrate great distances in galaxies similar to the Milky Way, potentially altering our view of habitable zones. This finding could change scientists' understanding of where and how life could evolve in a galaxy.
SourceUniversity of Washington·JournalThe Astrophysical Journal Letters·DateSep 15, 2008
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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.
SourceESO·JournalThe Astrophysical Journal Letters·DateAug 26, 2008
The Hubble Space Telescope has resolved individual threads of gas in the filaments of galaxy NGC 1275, revealing a magnetic structure that sustains them for over 100 million years. The discovery provides crucial clues about how giant black holes affect their surroundings.
SourceESA/Hubble Information Centre·JournalNature·DateAug 20, 2008
A Dutch school teacher, Hanny van Arkel, discovered a mysterious gaseous object with a hole in the center while classifying galaxy images on the Galaxy Zoo project. Scientists are now investigating this phenomenon, known as 'Hanny's Voorwerp,' which they believe could be a new class of astronomical object, possibly a quasar.
SourceYale University·JournalMonthly Notices of the Royal Astronomical Society·DateAug 5, 2008
Astronomers have tracked a recent supernova explosion in the Milky Way galaxy using NASA's Chandra X-ray Observatory and NRAO's VLA. The discovery confirms the supernova is about 140 years old, making it the youngest recorded in the galaxy.
SourceChandra X-ray Center·JournalThe Astrophysical Journal Letters·DateMay 14, 2008
A team of astronomers from Queen's University Belfast have discovered the nature of five supernova precursor stars using Hubble images. The study reveals that stars with masses as low as seven times the mass of the Sun can explode as supernovae, challenging current understanding of massive star collapse.
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The galaxy proto-cluster LBG-2377 is the farthest ever detected, offering a glimpse into the universe's infancy when its light was emitted. Scientists believe it may grow into a massive galaxy cluster, born from a catastrophic event with gas and matter collapsing.
The Large Binocular Telescope on Mount Graham achieved its first binocular light using twin side-by-side 8.4-meter primary mirrors, showcasing the telescope's power and clarity. The images reveal details of the spiral galaxy NGC 2770, including newly formed hot stars and older, cooler stars.
The Triangulum Galaxy, located 2.9 million light-years from Earth, is ablaze with starbirth, according to a new image taken by NASA's Swift satellite. The image showcases the galaxy's high spatial resolution, revealing young, hot stars and star-forming gas clouds in unprecedented detail.
Researchers have discovered a giant hydrogen gas finger in the Milky Way Galaxy, which may indicate that nearby galaxies, such as the Large and Small Magellanic Clouds, will eventually merge with our Galaxy. The study provides valuable insight into the galaxies' fate using CSIRO radio telescopes.
SourceCSIRO Australia·JournalThe Astrophysical Journal Letters·DateFeb 4, 2008
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Astronomers have determined that a hyperfast star, HE 0437-5439, originated from the Large Magellanic Cloud, contradicting its initial assumption of coming from the Milky Way. The star's elemental composition and velocity indicate it was ejected from the LMC by a massive black hole.
SourceCarnegie Institution for Science·JournalThe Astrophysical Journal Letters·DateJan 28, 2008
The Arecibo Observatory has discovered methanimine and hydrogen cyanide, two key ingredients for life, in a distant galaxy. These molecules were found by searching for radio emission at specific frequencies, using the world's largest and most sensitive radio telescope.
The Hubble Space Telescope has discovered a double Einstein ring, caused by the bending of light from two distant galaxies behind a massive foreground galaxy. The discovery offers insights into dark matter and the nature of distant galaxies.
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.
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Astronomers discover triple merger of galaxies, dubbed 'The Bird', with ESO's VLT. The system reveals two massive spiral galaxies and a third irregular galaxy forming stars at high rates.
SourceESO·JournalMonthly Notices of the Royal Astronomical Society·DateDec 20, 2007
Researchers solved a longstanding problem of the Cold Dark Matter cosmology model by exposing a critical relationship between interstellar gas and dark matter in galaxy birth. The study showed that dense gas clouds in galaxies form massive stars, which drive 'sloshing' effects that kick dark matter out of the galaxy's center.
A team from Rochester Institute of Technology has confirmed that supermassive black holes launch rotating winds that shape galaxies and regulate their growth. The findings, reported in Nature, provide direct observational confirmation of a long-standing theory about quasar winds.
SourceRochester Institute of Technology·JournalNature·DateOct 31, 2007
An international team of scientists has identified a tiny galaxy, about half the size and one-tenth the weight of the smallest distant galaxies typically observed. The galaxy is 100 times lighter than our own Milky Way and is 100 times closer to us than the nearest known structure, the Virgo cluster.
SourceUniversity of California - Santa Barbara·DateOct 4, 2007
The Hercules Dwarf Galaxy, a tiny companion to the Milky Way, has been found to have an exceptional flat shape, unlike any other known galaxy. The galaxy's shape is likely due to its close proximity to the Milky Way and the gravitational forces that disrupt it.
SourceMax-Planck-Gesellschaft·JournalThe Astrophysical Journal Letters·DateSep 14, 2007
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Astronomers have witnessed the rare sight of four galaxies crashing into each other, kicking up billions of stars and forming a single, massive galaxy. The merger, observed using NASA's Spitzer Space Telescope and WIYN Telescope, provides unprecedented insight into how the most massive galaxies in the universe form.
SourceYale University·JournalThe Astrophysical Journal Letters·DateAug 6, 2007
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.
SourceChandra X-ray Center·JournalThe Astrophysical Journal Letters·DateJul 24, 2007
Astronomers have observed two Type II and Type Ia supernovae exploding in the same galaxy just 16 days apart. The rare event is unlikely to be related to anything unusual about the galaxy.
Researchers used supercomputers to simulate galaxy mergers, revealing the formation of a new type of structure - a central disk of gas that can be thousands of light years wide. The simulations predict that the gas in this disk will extract energy from the orbiting black holes, causing them to merge and produce strong gravitational waves.
SourceStanford University·JournalScience·DateJun 7, 2007
The Hubble Space Telescope provides a detailed view of Messier 81, revealing young blue stars and glowing regions of fluorescent gas. The galaxy's central black hole is 15 times the mass of the Milky Way's black hole.
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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.
SourceUniversity of California - Riverside·JournalScience·DateMay 17, 2007
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.
A team of German astronomers has identified a new globular cluster in the Milky Way, comprising approximately 100,000 stars. The discovery is significant as it provides unique laboratory conditions to investigate various aspects of astrophysics and sheds light on the formation and evolution of galaxies.
SourceESO·JournalMonthly Notices of the Royal Astronomical Society·DateMar 13, 2007
The AEGIS survey reveals a consistent relation between galaxy mass and star and gas orbital speed over billions of years, constraining galaxy formation theories. The findings suggest fundamental properties of galaxies have changed little over the past 8 billion years.
SourceUniversity of California - Santa Cruz·JournalThe Astrophysical Journal Letters·DateMar 6, 2007
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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.