Dwarf Galaxy Caught Ramming into a Large Spiral
Shown here, observations from NASA's Chandra X-ray telescope reveal a massive cloud of multimillion-degree gas in a galaxy about 60 million light years from Earth. The hot gas cloud is likely caused by a collision between a dwarf galaxy [bottom left] and a much larger galaxy called NGC 1232 [center]. The image, which combines X-rays and optical light, shows the scene of the collision. Chandra X-ray data, in purple, show the hot gas has a comet-like appearance, caused by the motion of the dwarf galaxy. Optical data from the European Southern Observatory's Very Large Telescope reveal the spiral galaxy in blue and white. The X-ray emission source at the top right of the image appears to be unrelated to the galaxy collision. If confirmed, this discovery would mark the first time such a collision has been detected only in X-rays, and could have implications for understanding how galaxies grow through similar collisions. The impact between the dwarf galaxy and the spiral galaxy caused a shock wave—akin to a sonic boom on Earth—that generated the hot gas with a temperature of about 6 million degrees.
Used in 2014 Calendar.
Chandra X-ray data shows a hot gas cloud caused by colliding galaxies.
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Credits
Please give credit for this item to:
NASA/Chandra X-ray Observatory/Huntingdon Institute for X-ray Astronomy/G.Garmire/European Southern Observatory/Very Large Telescope
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Project support
- Mark Malanoski (Global Science and Technology, Inc.)
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Writer
- Heather Hanson (Global Science and Technology, Inc.)
Release date
This page was originally published on Friday, November 1, 2013.
This page was last updated on Thursday, October 10, 2024 at 12:21 AM EDT.