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For release: 08-19-03
Photo release #: 03-141

Chandra reveals X-ray flow in Horseshoe Nebula

Photo description: Chandra image of the Horseshoe Nebula Large 2250 x 2250 (300)
Medium 720 x 720 (72)
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M17: 'X-ray champagne flow' uncorked in Horseshoe Nebula

A new image from NASA's Chandra X-ray Observatory reveals hot gas flowing away from massive young stars in the center of the Horseshoe Nebula, also known as M17 or the Omega Nebula. A group of massive young stars responsible for the activity in the nebula is located in the bright pink region near the center of the image.

Chandra's resolving power enabled astronomers to separate the contribution of these and other stars in the nebula from X-rays produced by the hot gas flow, which is shown in red. Temperatures in the hot gas flow range from 1.5 million degrees Celsius (2.7 million degrees Fahrenheit) to about 7 million degrees Celsius (13 million degrees Fahrenheit). The blue color indicates areas where stars are embedded in clouds of dust and gas that absorb low energy X-rays.

An infrared image of the Horseshoe Nebula reveals a cloud of much cooler gas and dust shaped like a horseshoe that gives the nebula its name. The hot gas shown by the Chandra image fits inside the cool gas cloud, and appears to have formed the horseshoe shape by carving a cavity in the cool gas. This activity could lead to the formation of new stars in the Horseshoe.

The stars in the Horseshoe Nebula are only about a million years old, so the nebula is too young for one of its stars to have exploded as a supernova and heated the gas. Collisions between high-speed winds of particles flowing away from the massive stars could heat the gas, or the hot gas could be produced as these winds collide with cool clouds to form bubbles of hot gas. This hot gas appears to be flowing out of the Horseshoe like champagne flows out of a bottle when the cork is removed, so it has been termed an "X-ray champagne flow."

A comparison with other young star clusters confirms that massive young stars are responsible for hot gas clouds like the one seen in the Horseshoe Nebula. The Arches cluster, which contains many massive young stars shows this type of cloud, whereas the central regions of the Orion Nebula, which has few massive young stars, does not.

NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program for the Office of Space Science, NASA Headquarters, Washington. Northrop Grumman of Redondo Beach, Calif., formerly TRW, Inc., was the prime development contractor for the observatory. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center in Cambridge, Mass.

The image and additional information are available at:

http://chandra.harvard.edu
and
http://chandra.nasa.gov

(NASA/CXC/PSU/L.Townsley et al.)


Contact
Steve Roy
Media Relations Dept.
(256) 544-0034

Megan Watzke
Chandra X-ray Obs. Center
(617) 496-7998

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