An international team of astronomers has discovered a rare square galaxy with a striking resemblance to an emerald cut diamond within a group of 250 galaxies some 70 million light years away.
False-color image of the unusually shaped galaxy LEDA 074886 (Alister Graham et al.)
The discovery will be published in the Astrophysical Journal.
The unusually shaped galaxy, called LEDA 074886, was detected in a wide field-of-view image taken with the Japanese Subaru Telescope for an unrelated program by Dr. Lee Spitler, an astrophysicist at Swinburne University of Technology and a co-author of the paper.
“In the Universe around us, most galaxies exist in one of three forms: spheroidal, disc-like, or lumpy and irregular in appearance,” said Associate Professor Alister Graham of Swinburne University of Technology, a lead author of the paper. “The rare rectangular-shaped galaxy was a very unusual object. It’s one of those things that just makes you smile because it shouldn’t exist, or rather you don’t expect it to exist. It’s a little like the precarious Leaning Tower of Pisa or the discovery of some exotic new species which at first glance appears to defy the laws of nature.”
The astronomers suspect it is unlikely that this galaxy is shaped like a cube. Instead, they believe that it may resemble an inflated disc seen side on, like a short cylinder.
Support for this scenario comes from observations with the giant Keck Telescope in Hawaii, which revealed a rapidly spinning, thin disc with a side on orientation lurking at the center of the galaxy. The outermost measured edge of this galactic disc is rotating at a speed in excess of 100,000 kilometers per hour.
“One possibility is that the galaxy may have formed out of the collision of two spiral galaxies,” said Swinburne’s Professor Duncan Forbes, a co-author of the paper. “While the pre-existing stars from the initial galaxies were strewn to large orbits creating the emerald cut shape, the gas sank to the mid plane where it condensed to form new stars and the disc that we have observed.”
Despite its apparent uniqueness, partly due to its chance orientation, the astronomers have managed to glean useful information for modeling other galaxies.
While the outer boxy shape is somewhat reminiscent of galaxy merger simulations, which don’t involve the production of new stars, the disc-like structure is comparable with merger simulations involving star formation.
“This highlights the importance of combining lessons learned from both types of past simulation for better understanding galaxy evolution in the future,” explained Dr. Graham. “One of the reasons this emerald cut galaxy was hard to find is due to its dwarf-like status: it has 50 times less stars than our own Milky Way galaxy, plus its distance from us is equivalent to that spanned by 700 Milky Way galaxies placed end-to-end.”
“Curiously, if the orientation was just right, when our own disc-shaped galaxy collides with the disc-shaped Andromeda galaxy about three billion years from now we may find ourselves the inhabitants of a square looking galaxy,” the astronomer concluded.
Article source: http://www.sci-news.com/astronomy/article00218.html
Tags: Duncan Forbes, milky way galaxy, Associate Professor Alister Graham, Alister Graham <BR/>
