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New scientific riches from Integral
 
7 November 2007

The soft gamma-ray sky
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This image shows the soft gamma-ray sky, as revealed by Integral during its first five years of operation. Soft gamma rays each have energy somewhere between 20-100 keV. Most sources of celestial gamma ray in the Universe emit in this region of the gamma ray spectrum. This image is a mosaic of data taken with the Imager on Board the Integral Satellite (IBIS).

Credits: ESA/ Integral/ IBIS Survey Team
 
 
Artist's view of Integral
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Integral, ESA's International Gamma-Ray Astrophysics Laboratory, is gathering some of the most energetic radiation that comes from space. The spacecraft was launched in October 2002 and is helping to solve some of the biggest mysteries in astronomy.

Gamma rays are even more powerful than the X-rays used in medical examinations. Fortunately, Earth's atmosphere acts as a shield to protect us from this dangerous cosmic radiation. However this means that gamma rays from space can only be detected by satellites.

At time of launch, Integral was the most sensitive gamma-ray observatory ever put into space. It detects radiation from the most violent events far away and from processes that made the Universe habitable.

Credits: ESA

 
 
High-mass X-ray binaries
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This is an artist's impression of Integral’s investigation of high-mass X-ray binaries. Integral has revealed two different types of stars. In the first example (top panel), the neutron star companion is buried deeply in the extended outer envelope of the star. This results in persistent X-ray emission. In the second example (bottom panel), the neutron star only occasionally swallows material from the envelope, causing a sudden brightening of its gamma rays.

Credits: University of Paris (S. Chaty)
 


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Related ESA publications
Integral results leaflet (pdf)
In depth
Integral in-depth
 
 
 
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