Monday, 5 January 2015

"A Living Fossil from Early Universe" --Gigantic S-Shaped Dwarf Galaxy


In 2013, a UCLA team used a unique telescope to discover a previously unknown companion to the nearby galaxy NGC 4449 (image above), which is some 12.5 million light years from Earth. The newly discovered dwarf galaxy had escaped even the illuminating eyes of the Hubble Space Telescope. NGC 4449B is stretched into a gigantic "S" so large that if one end were placed at the center of the Milky Way, the other end would reach all the way to the sun's position. In fact, NGC 4449B is the largest dwarf galaxy known in the "local group" that also includes the Milky Way and the Andromeda galaxy.

The larger, host galaxy, NGC 4449, may be "something of a living fossil," representing what most galaxies probably looked like shortly after the Big Bang, Rich said. The galaxy is forming stars "so furiously" that it has giant clusters of young stars and even appears bluish — a sign of a young galaxy — to the eye in large amateur telescopes."

NGC 4449 has a nucleus that may someday host a black hole and an irregular structure, lacking the spiral arms characteristic of many galaxies, he said. It is surrounded by a huge complex of hydrogen gas that spans approximately 300,000 light years, which may be fueling its burst of star formation.

UCLA research astronomer Michael Rich collaborated with Francis Longstaff, a professor of finance at the UCLA Anderson School of Management and an amateur astronomer, in acquiring and using a specialized telescope designed to take images of wide fields of the sky. Known as the Centurion 28 (the diameter of the mirror is 28 inches), the telescope, and the observatory the astronomers used, are located at the Polaris Observatory Association.

With the C28 telescope, the astronomers discovered the companion dwarf galaxy, which has "evidently experienced a close encounter with the nucleus of NGC 4449," Rich said. Dubbed NGC 4449B, the dwarf galaxy has been stretched into a comet-like shape by this gravitational encounter.

NGC 4449B had remained undetected because it is more than 10 times fainter than the natural brightness of the night sky and some 1,000 times fainter than our own Milky Way galaxy. The dwarf galaxy is in a "transient stage," Rich said, and will soon — by astronomical standards — be dissolved. The Milky Way has a similar companion, known as the Sagittarius Dwarf galaxy, which has been wrapped around our galaxy as it orbits and which loses its stars to the Milky Way's gravitational tug.

With the help of the wide field of the C28 telescope and special image processing conducted by Christine Black, a UCLA research assistant, and David Reitzel of the Griffith Observatory, the astronomers were able to subtract the light of the sky and that of the outer parts of NGC 4449 to reveal the new galaxy.

The deep images of the larger NGC 4449 revealed other surprises as well: a strange arc of stars that might be an ingested galaxy, and a "remarkable halo" of old stars that appears to consist of two parts; the outermost part of this "halo" population was unexpected, and makes NGC 4449 equivalent in size to the Milky Way.

The origin of these old stars is not known, but they may have been acquired when galaxies similar to NGC 4449B fell into NGC 4449 and were shredded, Rich said.

"Our own galaxy, the Milky Way, has a host of smaller galaxies which orbit around it, " added Andrew Benson, a co-author and a senior research fellow in theoretical cosmology at the California Institute of Technology. "On much larger scales, we see groups and clusters of galaxies which orbit under the pull of their mutual gravitational attraction. Gravity has no preferred length scale, so we'd expect that dark matter (which interacts only through gravity) should behave in more or less the same way on all scales. For a galaxy like NGC4449, that means it should have its own system of small dark-matter satellites orbiting around it — assuming that dark matter works the way we think it does."

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