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Galactic Center Radio Arc

From Wikipedia, the free encyclopedia
X-ray filament in the galactic center that has a strong curve
Image of the Galactic Center Radio Arc. The bright source near the bottom right is thesupermassive black hole,Sagittarius A*at the center of theMilky Way galaxy.

TheGalactic Center Radio Arc is a long curvingX-ray filament about 40 light years across located in theGalactic Center of theMilky Way galaxy (about 8 kiloparsecs). TheCentral Molecular Zone (CMZ) also contains the Galactic central radio arc. The structure is curving towards the Galactic Center where thesupermassive black hole calledSagittarius A* is located.[1][2]

The curving is due to the hotplasma located inside the Galactic Center Radio Arc being directed and flowing along constant and strongmagnetic field lines.[1][3]

References

[edit]
  1. ^ab"APOD: 2023 April 3 – The Galactic Center Radio Arc".apod.nasa.gov. Retrieved2025-05-20.
  2. ^"Research Portal".iro.uiowa.edu.Archived from the original on 2025-04-17. Retrieved2025-05-20.
  3. ^Serabyn, E. (1996), Blitz, Leo; Teuben, Peter (eds.),"The Nature of the Galactic Center Arc",Unsolved Problems of the Milky Way: Proceedings of the 169th Symposium of the International Astronomical Union, held in the Hague, the Netherlands, August 23–29, 1994, Dordrecht: Springer Netherlands, pp. 263–269,doi:10.1007/978-94-009-1687-6_32,ISBN 978-94-009-1687-6, retrieved2025-05-20{{citation}}: CS1 maint: work parameter with ISBN (link)
Location
The Milky Way Galaxy
The Milky Way Galaxy
Structure
Galactic Center
Disk
Halo
Satellite
galaxies
Magellanic Clouds
Dwarfs
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