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Decade long study sheds light on "killer" galactic mergers

Decade long study sheds light on "killer" galactic mergers
Two merging galaxies known as Arp 302, also called VV 340
Two merging galaxies known as Arp 302, also called VV 340
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The merger of two galaxies, known as NGC 7752 (larger) and NGC 7753 (smaller), also collectively called Arp86
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The merger of two galaxies, known as NGC 7752 (larger) and NGC 7753 (smaller), also collectively called Arp86
The merger of two galaxies, known as NGC 6786 (right) and UGC 11415 (left), also collectively called VII Zw 96
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The merger of two galaxies, known as NGC 6786 (right) and UGC 11415 (left), also collectively called VII Zw 96
Two merging galaxies known as Arp 302, also called VV 340
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Two merging galaxies known as Arp 302, also called VV 340
View gallery - 3 images

Images taken by NASA's Spitzer Space telescope are providing insight into the phenomenon of "killer" galaxies that, when they merge, shut down star formation within the new united galaxies. The collision and mixing of a pair of galaxies under the right (or wrong) conditions can disrupt the processes that allow stars to form, effectively dooming the merged galaxy.

As Douglas Adams said, space is big – really big. There are trillions of galaxies spread throughout this vastness that form into clusters and some of them will interact with one another. Such interactions can be as benign as two galaxies passing or orbiting one another drawing out gases and distorting their rotating arms. Others can be high-speed collisions where the two galaxies pass through one another, or a larger one devours the smaller one.

And then there are galactic mergers where two galaxies of similar sizes collide with one another so slowly that they don't have enough momentum to separate again and form a new galaxy. These only happen in a small percentage of interactions, but NASA says that some of these can generate conditions that effectively shut down star formation, causing the new galaxy to die young as the older stars reach the end of their lives.

The merger of two galaxies, known as NGC 7752 (larger) and NGC 7753 (smaller), also collectively called Arp86
The merger of two galaxies, known as NGC 7752 (larger) and NGC 7753 (smaller), also collectively called Arp86

The Spitzer images are part of a decade-long study called the Great Observatories All-sky LIRG Survey (GOALS), which focused on looking at how galaxies merge. The survey of over 200 objects in our intergalactic neighborhood provided a number of examples of killer mergers. Since Spitzer operates in the infrared band of the spectrum, the images are rendered in false colors between 3.6 and 8.0 microns to bring out light emissions from both stars and interstellar dust.

According to NASA, when two galaxies merge, one of the perils is that the merged galaxy may end up with a supermassive black hole at the center that sucks most of the available gas and dust, preventing new stars from emerging. Another possibility is that the merger will generate shock waves from the giant black hole that will blow away gas and dust, again shutting down star formation.

The merger of two galaxies, known as NGC 6786 (right) and UGC 11415 (left), also collectively called VII Zw 96
The merger of two galaxies, known as NGC 6786 (right) and UGC 11415 (left), also collectively called VII Zw 96

This sounds very simple, but the space agency emphasizes that this is, in fact, a complex relationship that involves new bursts of star formation, the mechanics of black holes, and other processes. To better understand this, GOALS is working with both the Spitzer and the W.M. Keck Observatory in Hawaii to seek out shock waves in merging galaxies, which have been surprisingly lacking in one example under a detailed survey, indicating that more data is needed for a better understanding.

The GOALS program includes not only Spitzer, but also NASA's Hubble and Chandra space telescopes, the European Space Agency's Herschel satellite, the Keck Observatory, the National Science Foundation's Very Large Array, and the Atacama Large Millimeter Array.

Source: NASA

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