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Showing posts with label milky way. Show all posts
Showing posts with label milky way. Show all posts

Neighboring Galaxies Collided 2-3 Billion Years Ago

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An international team of astronomers, including Queen's University physicist Larry Widrow, have uncovered evidence of a nearby cosmic encounter. Their study indicates that the Andromeda and Triangulum galaxies, the two galaxies closest to our own, collided about two to three billion years ago.



              **The possible orbit of the Triangulum galaxy around Andromeda. (Credit: Image courtesy of Queen's University)**

"The encounter forever changed the structure of the galaxies," says Dr. Widrow, a professor of Physics, Engineering Physics and Astronomy at Queen's. "The collision between the galaxies appears to have caused millions of stars to be ripped from the Triangulum disk to form a faint stream visible in the PAndAS data."


Dr. Widrow, along with John Dubinsky of the University of Toronto, recreated this galactic encounter using a high performance computer and theoretical modeling. Their simulations illustrate how the strong gravitational field of Andromeda could have pulled stars away from the Triangulum disk creating a stream just as the team saw.

The Pan-Andromeda Archeological Survey (PAndAS), led by Alan McConnachie of the Herzberg Institute of Astrophysics in Victoria BC, is using the Canada-France-Hawaii telescope to map the Andromeda and Triangulum galaxies. This map, the largest of its kind, will allow astronomers to test the hypothesis that galaxies grow by "cannibalizing" other galaxies. The findings from the first year of the survey are published this week in the journal Nature. Galaxies are large collections of stars, often distributed in a disk-like pattern with spiral arms. Nearly 40 years ago, astronomers learned that galaxies are embedded in extended halos of dark matter.


"Our observations now show that stars also inhabit these outer halos," says Dr. Widrow. "We believe that these stars are relics of small galaxies that were destroyed by the powerful tidal fields of a larger galaxy. Our observations also suggest that the Triangulum Galaxy is being ripped apart by Andromeda."

Andromeda, and our own galaxy the Milky Way, are the two largest members of a small cluster of galaxies known as the Local Group. Triangulum, the third largest member of the Local Group, is about one-tenth the size of Andromeda.


"Within a few billion years Triangulum will be completely destroyed by Andromeda and its stars will be dispersed throughout the Andromeda halo," says Dr. Widrow. "And a few billion years after that, Andromeda and the Milky Way will collide and merge together to form a giant elliptical galaxy."


Source: AstronomyNow


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The Milky Way's Look Alike

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A new image from the European Southern Observatory (ESO) reveals an edge-on galaxy much like our own Milky Way.
 



**Seen edge-on, NGC 4945 appears much like our own Milky Way Galaxy. Sites of active star formation – HII regions – appear pink in this image. The field of view is 30 x 30 arcminutes; north is up and east is left. Image: ESO**

Taken with the Wide Field Imager (WFI) instrument on the 2.2 metre MPG/ESO telescope at the La Silla Observatory in Chile, the image of NGC 4945 reveals a spiral galaxy with swirling arms and a bar shaped central region resembling our home galaxy the Milky Way. But NGC 4945 has a brighter centre that likely hosts a supermassive black hole which is gorging on stellar matter and burping energy out into space. 


Astronomers classify NGC 4945 as a Seyfert galaxy, after American astronomer Carl Seyfert, who first identified this family of galaxies – a subclass of active galactic nuclei – to have curious light signatures emanating from their central engines. These emissions come from gas and dust falling into a disc around the black hole, which accelerates and heats it up until it emits high energy radiation such as X-rays and ultraviolet light. Most large spiral galaxies, including the Milky Way, host a black hole in their cores, though many of these monsters are at a stage of their lives where they no longer actively feed.

NGC 4945 resides 13 million light years from Earth in the constellation of Centaurs, and can be seen in modest amateur telescopes. It appears cigar-shaped from our perspective but it is actually many times wider than it is thick, with bands of stars and glowing gas marching around its centre. With the use of special optical filters to isolate the colour of light emitted by heated gases such as hydrogen, the new image from ESO displays sharp contrasts in NGC 4945 that indicate active areas of star formation. 
 

Source: AstronomyNow


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New Galaxy with Most Distant Supermassive Black Hole

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University of Hawaii astronomer Tomotsugu Goto and colleagues have discovered a giant galaxy surrounding the most distant black hole ever found. The galaxy, which is 12.8 billion light-years from Earth, is as large as the Milky Way galaxy and harbors a supermassive black hole that contains at least a billion times as much matter as does our Sun.

** False-color image of the QSO (CFHQSJ2329-301), the most distant black hole currently known. In addition to the bright central black hole (white), the image shows the surrounding host galaxy (red). Tomotsugu Goto, University of Hawaii**

"It is surprising that such a giant galaxy existed when the universe was only one-sixteenth of its present age, and that it hosted a black hole one billion times more massive than the Sun," Goto said. "The galaxy and black hole must have formed very rapidly in the early universe."

Knowledge of the host galaxies of supermassive black holes is important to understand the long-standing mystery of how galaxies and black holes have evolved together. Until now, studying host galaxies in the distant universe has been extremely difficult because the blinding bright light from the vicinity of the black hole makes it more difficult to see the already faint light from the host galaxy.

Unlike smaller black holes, which form when a large star dies, the origin of supermassive black holes remains an unsolved problem. A currently favored model requires several intermediate black holes to merge. The host galaxy discovered in this work provides a reservoir of such intermediate black holes. After forming, supermassive black holes often continue to grow because their gravity draws in matter from surrounding objects. The energy released in this process accounts for the bright light that these black holes produce.
To see the supermassive black hole, the team of scientists used new red-sensitive CCDs installed in the Suprime-Cam camera on the Subaru telescope on Mauna Kea. Satoshi Miyazaki of the National Astronomy Observatory of Japan (NAOJ) is lead investigator for the creation of the new CCDs and a collaborator on this project. "The improved sensitivity of the new CCDs has brought an exciting discovery as its very first result," Miyazaki said

A careful analysis of the colors revealed that 40 percent of light around 9100 angstroms is from the host galaxy itself and 60 percent is from the surrounding ionized nebulae illuminated by the black hole.

"We have witnessed a supermassive black hole and its host galaxy forming together," said Yousuke Utsumi from the Graduate University for Advanced Studies/NAOJ and a member of the project team. "This discovery has opened a new window for investigating galaxy-black hole co-evolution at the dawn of the universe."


 
Source: Univ. of Hawaii at Manoa's Institute


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