Jump to content

Portal:Radiation astronomy/Resource/38

From Wikiversity

High-velocity galaxies

[edit | edit source]
The irregular galaxy NGC 1427A is passing through the Fornax cluster at nearly 600 kilometers per second (400 miles per second). Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA).

"The irregular galaxy NGC 1427A is a spectacular example of the resulting stellar rumble. Under the gravitational grasp of a large gang of galaxies, called the Fornax cluster, the small bluish galaxy is plunging headlong into the group at 600 kilometers per second or nearly 400 miles per second."[1]

"Galaxy clusters, like the Fornax cluster, contain hundreds or even thousands of individual galaxies. Within the Fornax cluster, there is a considerable amount of gas lying between the galaxies. When the gas within NGC 1427A collides with the Fornax gas, it is compressed to the point that it starts to collapse under its own gravity. This leads to formation of the myriad of new stars seen across NGC 1427A, which give the galaxy an overall arrowhead shape that appears to point in the direction of the galaxy's high-velocity motion."[1]

References

[edit | edit source]
  1. 1.0 1.1 M. Gregg (3 March 2005). The Impending Destruction of NGC 1427A. Baltimore, Maryland USA: Hubblesite.org. http://hubblesite.org/newscenter/archive/releases/2005/09/image/a/. Retrieved 2016-11-05.