Mostrando entradas con la etiqueta Abell 1689. Mostrar todas las entradas
Mostrando entradas con la etiqueta Abell 1689. Mostrar todas las entradas

martes, 7 de enero de 2014

NASA : AAS Meeting Highlights Several New Hubble Science Findings


This composite of Hubble images was taken in visible and near-infrared light.
This composite of Hubble images was taken in visible and near-infrared light. Four unusually red objects (circled) appear as they existed just 500 million years after the big bang.
Image Credit: NASA/ESA/Illingworth,Oesch,UC-SC/Bouwens, Labb,Leiden U.
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NASA's Hubble Space Telescope is providing a new perspective on the remote universe, including new views of young and distant galaxies bursting with stars. Scientists described the findings Tuesday in a news conference sponsored by the American Astronomical Society (AAS).

Highlighted in the briefing were three discoveries -- four unusually bright galaxies as they appeared 13 billion years ago, the deepest image ever obtained of a galaxy cluster, and a sampling of galaxies thought to be responsible for most of the stars we see today.
The ultra-bright, young galaxies, discovered using data from NASA's Hubble and Spitzer space telescopes, are bursting with star formation activity, which accounts for their brilliance. The brightest one is forming stars approximately 50 times faster than our Milky Way galaxy does today. These fledgling galaxies are only one-twentieth the size of the Milky Way, but they probably contain about 1 billion stars crammed together.
Although Hubble has previously identified galaxies at this early epoch, astronomers were surprised to find objects that are about 10 to 20 times more luminous than anything seen previously.
"These just stuck out like a sore thumb because they are far brighter than we anticipated," explained Garth Illingworth of the University of California at Santa Cruz. "There are strange things happening regardless of what these sources are. We're suddenly seeing luminous, massive galaxies quickly build up at such an early time. This was quite unexpected."
The galaxies were first detected with Hubble. Its sharp images are crucial to finding such distant galaxies and enabled the astronomers to measure their star-formation rates and sizes. Using Spitzer, the astronomers were able to estimate the stellar masses by measuring the total stellar luminosity of the galaxies.
"This is the first time scientists were able to measure an object's mass at such a huge distance," said Pascal Oesch of Yale University in New Haven, Conn. "It's a fabulous demonstration of the synergy between Hubble and Spitzer."
The result bodes well for NASA's James Webb Space Telescope, currently in development. Scientists anticipate using Webb to look even farther back in time to find young, growing galaxies as they existed only a few hundred million years after the universe began in theorized big bang.
An unprecedented long distance view of the universe comes from an ambitious collaborative project with Hubble called The Frontier Fields. It is the longest and deepest exposure obtained to date of a cluster of galaxies, and shows some of the faintest and youngest galaxies ever detected. The image contains several hundred galaxies as they looked 3.5 billion years ago.
Galaxy Cluster Abell 1689
Astronomers used Hubble and the magnification power of the giant cluster of galaxies Abell 1689 to find 58 remote galaxies. They are the smallest, faintest, and most numerous galaxies ever seen in the remote universe.
Image Credit: NASA/ESA/B.Siana, A.Alavi, UC Riverside
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Appearing in the foreground of the image is Abell 2744, a massive galaxy cluster located in the constellation Sculptor. The immense gravity in Abell 2744 is being used as a lens to warp space and brighten and magnify images of more distant background galaxies. The more distant galaxies appear as they did longer than 12 billion years ago, not long after the big bang.
The Hubble exposure reveals almost 3,000 of these background galaxies interleaved with images of hundreds of foreground galaxies in the cluster. Their images not only appear brighter, but also smeared, stretched and duplicated across the field. Because of the gravitational lensing phenomenon, the background galaxies are magnified to appear as much as 10 to 20 times larger than they would normally appear. Furthermore, the faintest of these highly magnified objects is 10 to 20 times fainter than any galaxy observed previously. Without the boost from gravitational lensing, the many background galaxies would be invisible.
The Hubble exposure will be combined with images from Spitzer and NASA's Chandra X-ray Observatory to provide new insight into the origin and evolution of galaxies and their accompanying black holes.
Hubble also uncovered a substantial population of 58 young, diminutive galaxies that scientists long suspected were responsible for producing a majority of stars now present in the cosmos during the universe's early years.
Deep exposures in ultraviolet light, made with Hubble's Wide Field Camera 3, revealed a sampling of galaxies that existed more than 10 billion years ago, when the universe was roughly 3.4 billion years old. They are the smallest, faintest, galaxies seen in the remote universe to date. A census of galaxies existing at the time indicates these small, faint galaxies are 100 times more abundant in the universe than their more massive cousins.
"There's always been a concern that we've only found the brightest of the distant galaxies," said Brian Siana of the University of California at Riverside. "The bright galaxies, however, represent the tip of the iceberg. We believe most of the stars forming in the early universe are occurring in galaxies we normally can't see at all. Now we have found those 'unseen' galaxies, and we're really confident that we're seeing the rest of the iceberg."
Hubble Frontier Field Abell 2744
This long-exposure Hubble Space Telescope image of massive galaxy cluster Abell 2744 (foreground) is the deepest ever made of any cluster of galaxies. It shows some of the faintest and youngest galaxies ever detected in space.
Image Credit: NASA/ESA/J.Lotz, M.Mountain, A.Koekemoer/STScI HFF Team
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Normally too faint for Hubble to see, these galaxies were revealed through gravitational lensing focused on a massive galaxy cluster known as Abell 1689 in the constellation Ursa Major. The cluster magnified light emitted by distant objects behind it, causing the newly discovered galaxies to appear bigger and brighter. If this sample is representative of the entire population at the time, then the majority of new stars formed in such small, unseen galaxies.
"Though these galaxies are very faint, their increased numbers mean that they account for the majority of star formation during this epoch," said team member Anahita Alavi, also of the University of California at Riverside.
The astronomers were surprised to find the deeper they looked with Hubble, the more faint galaxies they found.
"Our goal with these observations was not to find a large number of galaxies, but to find much fainter galaxies," said Alavi.
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Guillermo Gonzalo Sánchez Achutegui

domingo, 15 de septiembre de 2013

NASA - Hubble Uncovers Largest Known Group of Star Clusters, Clues to Dark Matter


Globular Clusters in Abell 1689 Galaxy Grouping
Hubble Space Telescope image of largest known population of globular clusters, in Abell 1689 galaxy grouping. Image Credit: NASA/ESA
NASA's Hubble Space Telescope has uncovered the largest known population of globular star clusters, an estimated 160,000, swarming like bees inside the crowded core of the giant grouping of galaxies known as Abell 1689.
An international team of astronomers used Hubble's Advanced Camera for Surveys to discover this bounty of stellar fossils and confirm such compact groupings can be used as reliable tracers for dark matter, the invisible gravitational scaffolding on which galaxies are built.
"We show how the relationship between globular clusters and dark matter depends on the distance from the center of the galaxy grouping," Karla Alamo-Martinez of the Center for Radio Astronomy and Astrophysics of the National Autonomous University of Mexico in Morelia. "In other words, if you know how many globular clusters are within a certain distance, we can give you an estimate of the amount of dark matter."
Alamo-Martinez is lead author of a paper on the findings published online Sept. 10 and appearing in the Sept. 20 print edition of The Astrophysical Journal, and part of a team led by John Blakeslee of National Research Council Canada's Herzberg Institute of Astrophysics at the Dominion Radio Astrophysical Observatory in Victoria, British Columbia.
Globular clusters, dense bunches of hundreds of thousands of stars, are the homesteaders of galaxies. They contain some of the oldest surviving stars in the universe. Almost 95 percent of globular cluster formation occurred within the first 1 billion to 2 billion years after our universe was born in the theorized Big Bang 13.8 billion years ago.
Studying globular clusters is critical to understanding the early, intense star-forming events that mark galaxy formation. Understanding dark matter can yield clues on how large structures such as galaxies and galaxy clusters were assembled billions of years ago.
The globular star cluster in Abell 1689 is roughly twice as large as any other population found in previous globular cluster surveys -- in comparison, our Milky Way galaxy hosts about 150 -- and constitutes the most distant such systems ever studied, at 2.25 billion light-years away. The Hubble study shows most of the globular clusters in Abell 1689 formed near the center of the galaxy grouping, which contains a deep well of dark matter. The farther away from the galaxy core Hubble looked, the fewer globular clusters it detected. This observation corresponded with a comparable drop in the amount of dark matter, based on previous research.
"The globular clusters are fossils of the earliest star formation in Abell 1689, and our work shows they were very efficient in forming in the denser regions of dark matter near the center of the galaxy cluster," Blakeslee said. "Our findings are consistent with studies of globular clusters in other galaxy clusters, but extend our knowledge to regions of higher dark matter density."
Peering deep inside the heart of Abell 1689, Hubble detected the visible-light glow of 10,000 globular clusters, some as dim as 29th magnitude, which is 1 one-billionth the faintness of the dimmest star that can be seen with the naked eye. Based on that number, Blakeslee's team estimated that more than 160,000 globular clusters are huddled within a diameter of 2.4 million light-years.
"Even though we are looking deep into the cluster, we're only seeing the brightest globular clusters, and only near the center of Abell 1689 where Hubble was pointed," he said.
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Guillermo Gonzalo Sánchez Achutegui
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