Milky Way

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Vast cloud of antimatter traced to binary stars

Four years of observations from the European Space Agency’s Integral (INTErnational Gamma-Ray Astrophysics Laboratory) satellite may have cleared up one of the most vexing mysteries in our Milky Way: the origin of a giant cloud of antimatter surrounding the galactic center.

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Astronomy teams discover ancestors of Milky Way-type galaxies

Astronomers at Rutgers and Penn State universities have discovered galaxies in the distant universe that are ancestors of spiral galaxies like our Milky Way.

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New population of faint protogalaxies discovered

Astronomers have found a new population of faint protogalaxies by taking the most sensitive spectroscopic survey ever of a time when the universe was only 15% of its present age. These objects are the probable building blocks of galaxies today, including our own Milky Way.

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From molecules to Milky Way

Most people have a few gigabytes of files on their PC. In the next decade, astronomers expect to be processing 10 million gigabytes of data every hour from the Square Kilometre Array telescope.

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Extreme star cluster bursts into life in new Hubble image

The NASA/ESA Hubble Space Telescope has captured a spectacular image of NGC 3603, a giant nebula hosting one of the most prominent massive young clusters in the Milky Way, thus supplying a prime template for star formation studies.

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Why is Hercules Dwarf Galaxy so flat?

Through some of very first scientific observations with the brand-new Large Binocular Telescope in Arizona, an international team of astronomers has found that recently discovered tiny companion galaxy to our Milky Way, named Hercules Dwarf Galaxy, has truly exceptional properties: while basically all of its known peers in realm of these tiny dwarf galaxies are rather round, this galaxy at distance of 430,000 Light Years appears highly flattened, either shape of disk or of cigar.

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Brother for Milky Way's black hole

IS A second black hole lurking at the heart of the Milky Way? A relatively simple test could answer the question: look for a pair of stars fleeing the galaxy at breakneck speed.

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How supermassive black holes bind into pairs during galaxy mergers

Picture the Milky Way galaxy-a disk of stars and gas, a stellar spheroid and an enormous halo of dark matter. It spirals around a black hole that is supermassive-about three million solar masses. The Milky Way's total mass is about 100 billion solar masses-enormous to us but average among galaxies.

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Adaptive optics leads way to supermassive black holes

Astronomers have discovered the exact location and makeup of a pair of supermassive black holes at the center of a collision of two galaxies more than 300 million light years away.

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New technique for 'weighing' black holes

ESA's XMM-Newton has helped to find evidence for the existence of controversial Intermediate Mass Black Holes. Scientists used a new, recently proven method for determining the mass of black holes.

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Chemical Composition of Stars Can Tell History of our Galaxy

Using ESO's Very Large Telescope, an international team of astronomers has shown how to use the chemical composition of stars in clusters to shed light on the formation of our Milky Way. This discovery is a fundamental test for the development of a new chemical tagging technique uncovering the birth and growth of our Galactic cradle.

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New Globular Cluster Found in Milky Way

Images made with ESO's New Technology Telescope at La Silla by a team of German astronomers reveal a rich circular cluster of stars in the inner parts of our Galaxy. Located 30,000 light-years away, this previously unknown closely-packed group of about 100,000 stars is most likely a new globular cluster.

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