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Subject: Green Bank Telescope Reveals Satellite of Milky Way in Retrograde
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National Radio Astronomy Observatory
520 Edgemont Road
Charlottesville, VA 22903
http://www.nrao.edu

Contact:

Charles Blue, Public Information Officer, Charlottesville, VA
(434) 296-0323, cblue@nrao.edu

For Release: Thursday, May 22, 2003

GBT Reveals Satellite of Milky Way in Retrograde Orbit

New observations with National Science Foundation's Robert C. Byrd Green 
Bank Telescope (GBT) suggest that what was once believed to be an 
intergalactic cloud of unknown distance and significance, is actually a 
previously unrecognized satellite galaxy of the Milky Way orbiting 
backward around the Galactic center.

Jay Lockman of the National Radio Astronomy Observatory (NRAO) in Green 
Bank, West Virginia, discovered that this object, known as "Complex H," 
is crashing through the outermost parts of the Milky Way from an 
inclined, retrograde orbit. Lockman's findings will be published in the 
July 1 issue of the Astrophysical Journal, Letters.

"Many astronomers assumed that Complex H was probably a distant neighbor 
of the Milky Way with some unusual velocity that defied explanation," 
said Lockman. "Since its motion appeared completely unrelated to 
Galactic rotation, astronomers simply lumped it in with other high 
velocity clouds that had strange and unpredictable trajectories."

High velocity clouds are essentially what their name implies, 
fast-moving clouds of predominately neutral atomic hydrogen. They are 
often found at great distances from the disk of the Milky Way, and may 
be left over material from the formation of our Galaxy and other 
galaxies in our Local Group. Over time, these objects can become 
incorporated into larger galaxies, just as small asteroids left over 
from the formation of the solar system sometimes collide with the Earth.

Earlier studies of Complex H were hindered because the cloud currently 
is passing almost exactly behind the outer disk of the Galaxy. The 
intervening dust and gas that reside within the sweeping spiral arms of 
the Milky Way block any visible light from this object from reaching the 
Earth. Radio waves, however, which have a much longer wavelength than 
visible light, are able to pass through the intervening dust and gas.

The extreme sensitivity of the recently commissioned GBT allowed Lockman 
to clearly map the structure of Complex H, revealing a dense core moving 
on an orbit at a 45-degree angle to the plane of the Milky Way. 
Additionally, the scientist detected a more diffuse region surrounding 
the central core. This comparatively rarefied region looks like a tail 
that is trailing behind the central mass, and is being decelerated by 
its interaction with the Milky Way.

"The GBT was able to show that this object had a diffuse 'tail' trailing 
behind, with properties quite different from its main body," said 
Lockman. "The new data are consistent with a model in which this object 
is a satellite of the Milky Way in an inclined, retrograde orbit, whose 
outermost layers are currently being stripped away in its encounter with 
the Galaxy."

These results place Complex H in a small club of Galactic satellites 
whose orbits do not follow the rotation of the rest of the Milky Way. 
Among the most prominent of these objects are the Magellanic Clouds, 
which also are being affected by their interaction with the Milky Way, 
and are shedding their gas in a long stream.

Since large galaxies, like the Milky Way, form by devouring smaller 
galaxies, clusters of stars, and massive clouds of hydrogen, it is not 
unusual for objects to be pulled into orbit around the Galaxy from 
directions other than that of Galactic rotation.

"Astronomers have seen evidence that this accreting material can come in 
from wild orbits," said Butler Burton, an astronomer with the NRAO in 
Charlottesville, Virginia. "The Magellanic clouds are being torn apart 
from their interaction with the Milky Way, and there are globular 
clusters rotating the wrong way. There is evidence that stuff was going 
every-which-way at the beginning of the Galaxy, and Complex H is 
probably left over from that chaotic period."

The new observations place Complex H at approximately 108,000 
light-years from the Galactic center, and indicate that it is nearly 
33,000 light-years across, containing approximately 6 million solar 
masses of hydrogen.

Radio telescopes, like the GBT, are able to observe these cold, dark 
clouds of hydrogen because of the natural electromagnetic radiation 
emitted by neutral atomic hydrogen at radio wavelengths (21 centimeters).

Globular clusters, and certain other objects in the extended Galactic 
halo, can be studied with optical telescopes because the material in 
them has collapsed to form hot, bright stars.

The GBT is the world's largest fully steerable radio telescope. It was 
commissioned in August of 2000, and continues to be outfitted with the 
sensitive receivers and components that will allow it to make 
observations at much higher frequencies.

The National Radio Astronomy Observatory is a facility of the National 
Science Foundation, operated under cooperative agreement by Associated 
Universities, Inc.

IMAGE CAPTION:
[http://www.nrao.edu/pr/2003/complexh/cmpxh.jpg (436KB)]
Artist's rendition of the path of satellite galaxy Complex H (in red) in 
relation to the orbit of the Sun (in yellow) about the center of the 
Milky Way Galaxy. The outer layers of Complex H are being stripped away 
by its interaction with the Milky Way. The hydrogen atmosphere (in blue) 
is shown surrounding the visible portion (in white) of the Galaxy. 
CREDIT: Lockman, Smiley, Saxton; NRAO/AUI


