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NGC 6872: Galaxy Collision Switches on Black Hole

  • NGC 6872 and IC 4970 are two galaxies in the process of merging

  • IC 4970 is the small galaxy at the top of the image that, thanks to Chandra and Spitzer data, is shown to contain an active supermassive black hole

  • It was puzzling where IC 4970 got its fuel supply since observations reveal a lack of material surrounding the black hole

  • The new results show IC 4970 has stripped cold gas from NGC 6872 and is using it to feed its growing black hole

This composite image of data from three different telescopes shows an ongoing collision between two galaxies, NGC 6872 and IC 4970 (roll your mouse over the image above). X-ray data from NASA's Chandra X-ray Observatory is shown in purple, while Spitzer Space Telescope's infrared data is red and optical data from ESO's Very Large Telescope (VLT) is colored red, green and blue.

Astronomers think that supermassive black holes exist at the center of most galaxies. Not only do the galaxies and black holes seem to co-exist, they are apparently inextricably linked in their evolution. To better understand this symbiotic relationship, scientists have turned to rapidly growing black holes - so-called active galactic nucleus (AGN) - to study how they are affected by their galactic environments.

The latest data from Chandra and Spitzer show that IC 4970, the small galaxy at the top of the image, contains an AGN, but one that is heavily cocooned in gas and dust. This means in optical light telescopes, like the VLT, there is little to see. X-rays and infrared light , however, can penetrate this veil of material and reveal the light show that is generated as material heats up before falling onto the black hole (seen as a bright point-like source).

Despite this obscuring gas and dust around IC 4970, the Chandra data suggest that there is not enough hot gas in IC 4970 to fuel the growth of the AGN. Where, then, does the food supply for this black hole come from? The answer lies with its partner galaxy, NGC 6872. These two galaxies are in the process of undergoing a collision, and the gravitational attraction from IC 4970 has likely pulled over some of NGC 6872's deep reservoir of cold gas (seen prominently in the Spitzer data), providing a new fuel supply to power the giant black hole.

Fast Facts for NGC 6872:
Credit  X-ray: NASA/CXC/SAO/M.Machacek; Optical: ESO/VLT; Infrared: NASA/JPL/Caltech
Release Date  December 10, 2009
Scale  Image is 347 arcsec across (310,000 light years)
Category  Normal Galaxies & Starburst Galaxies
Coordinates (J2000)  RA 20h 16m 57s | Dec -70 46' 06
Constellation  Pavo
Observation Date  December 14 & 16, 2005
Observation Time  21 hours
Obs. ID  7248, 7059
Instrument  ACIS
References Machacek, et al., 2008 ApJ 674 142-150
Color Code  X-ray (Purple); Optical (Red, Green, Blue); Infrared (Dark Red)
IR
Optical
X-ray
Distance Estimate  About 180 million light years
Visitor Comments (4)

Entranced by Science and Discovery and Nat Geo channels. But can you get a bit of time on evening news so that the wondrous things happening in our own universe can be understood or at least the words can be in more people's memory banks. Just a little news is better than none. Thanks C.

Posted by Carolyn Neuman on Tuesday, 10.16.12 @ 14:00pm


Thanks for your question. The collision has already started and will continue for many millions of years.

P. Edmonds for CXC

Posted by P. Edmonds on Wednesday, 03.3.10 @ 10:50am


Is there an estimation in time about when the collision will take place?
Regards De Mitri M

Posted by Maurizio De Mitri - Italy on Thursday, 02.18.10 @ 04:59am


I know that the process of galactic collisions take a very long time. What is the evidences that, told you that these two are in the process of colliding?

Marvin L. S.

Posted by Marvin L. S. on Friday, 12.11.09 @ 01:29am


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