Two Stars, One Powerful Glow
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- Visualizations by:
- Scott Wiessinger
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- Written by:
- Francis Reddy
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- Produced by:
- Scott Wiessinger
- View full credits
Using data from NASA's Fermi Gamma-ray Space Telescope and other facilities, an international team of scientists has found the first gamma-ray binary in another galaxy and the most luminous one ever seen. The dual-star system, dubbed LMC P3, lies within the expanding debris of a supernova explosion located in the Large Magellanic Cloud, a small nearby galaxy about 163,000 light-years away. The system contains a massive star and a crushed stellar core that interact to produce a flood of gamma rays, the highest-energy form of light. In gamma-ray binaries, outflows from both stars collide and accelerate electrons to near the speed of light. When these particles collide with the star's visible light, it receives a boost up to gamma-ray levels. Fermi observations show gamma-ray output from LMC P3 changes as the companion orbits the star. This variation lets astronomers study many of the emission processes common to other gamma-ray sources in unique detail. Watch the video to learn more.
For More Information
See NASA.gov
Credits
Please give credit for this item to:
NASA's Goddard Space Flight Center
Gamma-ray sky map courtesy of NASA/DOE/Fermi LAT Collaboration
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Animator
- Scott Wiessinger (KBR Wyle Services, LLC) [Lead]
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Writer
- Francis Reddy (University of Maryland College Park) [Lead]
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Producer
- Scott Wiessinger (KBR Wyle Services, LLC) [Lead]
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Project support
- Francis Reddy (University of Maryland College Park)