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Integral: Stellar winds colliding at our cosmic doorstep 
ESA’s Integral has made the first unambiguous discovery of high-energy X-rays coming from a rare massive star at our cosmic doorstep, Eta Carinae. It is one of the most violent places in the galaxy, producing vast winds of electrically-charged particles colliding at speeds of thousands of kilometres per second. The only astronomical object that emits gamma-rays and is observable by the naked eye, Eta Carinae is monstrously large, so large that astronomers call it a hypergiant. It contains between 100–150 times the mass of the Sun and glows more brightly than four million Suns put together. Astronomers know that it is not a single star, but a binary, with a second massive star orbiting the first. It has long been suspected that such massive binary stars should give off high-energy X-rays, but until now, the instruments required for the observations were lacking. Recently, Integral has conclusively shown that Eta Carinae gives off high-energy X-rays, more or less in agreement with theoretical predictions.
The high-energy X-rays come from a vast shockwave, set up and maintained between the two massive stars. The shockwave is produced when the two stars’ stellar winds collide, creating a system that astronomers term a colliding-wind binary. Massive stars are constantly shedding particles that are ‘blown’ away into space by the effect of light and other radiation given off by the star. This starlight is so fierce that the stellar winds can reach speeds of 1500–2000 km/s. With two massive stars in close proximity, as they are in the Eta Carinae system, the winds collide and set up fearsome shockwaves where temperatures reach several thousand million degrees Kelvin. “It’s a very tough environment,” says Leyder.
Understanding this emission is important because astronomers believe that it lies at the heart of many diverse phenomena in the universe. Stellar winds have profound implications on the evolution of stars, the chemical evolution of the universe and as a source of energy in the galaxy. Massive stars are rare, so two in a binary system is even rarer. “In our galaxy, there are probably only 30-50 colliding-wind binaries that display a clear signature of wind-wind collision,” says Leyder. A year ago, ESA’s XMM-Newton saw X-rays from the colliding wind binary, HD 5980, situated in the neighbouring galaxy, the Small Magellanic Cloud.
To have a rare, massive binary star such as Eta Carinae virtually at our cosmic doorstep at 8000 light-years, close enough to be observable in detail, is a stroke of luck. Now that they know what to look for, astronomers will continue searching for other examples of colliding wind binaries emitting high-energy X-rays further afield. Notes for editors: ‘Hard X-ray Emission from Eta Carinae’ by J-C. Leyder, R. Walter and G. Rauw has been accepted for publication in the journal Astronomy and Astrophysics. For more information on XMM-Newton’s Colliding Wind Binary observation, see: First X-ray detection of a colliding-wind binary beyond the Milky Way For more information: Jean-Christophe Leyder, Institut d’Astrophysique et de Géophysique, Université de Liège, Belgium Email: Leyder @ astro.ulg.ac.be Roland Walter, Integral Science Data Centre, Observatoire de Genève, Switzerland Email : Roland.Walter @ obs.unige.ch Christoph Winkler, ESA Integral Project Scientist Email: Christoph.Winkler @ esa.int
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Integral anniversary (http://www.esa.int/SPECIALS/ESApod/SEMDFPAMS7F_0.html)