Most galaxies, including our own, have a huge but well-behaved black hole at their heart, while some have messy eaters that suck in vast amounts of matter that then shines brightly as it falls towards oblivion. This causes the telltale bright spots at the center of galaxies known as active galactic nuclei (AGN). Why are the two types so different? Until now, the leading theory has been that mergers between galaxies are instrumental in driving matter into the black holes, making them grow.
In a new study, the largest of its kind so far, astronomers set up an identity parade of galaxies to test this theory. Comparing 140 active galaxies with a control group of over 1,200 comparable inactive galaxies, they found that there has been no significant link between AGN activity and galactic mergers for at least the past 8 billion years. Therefore, other phenomena, such as instabilities within galaxies, collisions of molecular clouds, or tidal disruption by other galaxies flying by, must be to blame.
The emission of radiation from AGNs is driven by the behavior of matter, such as gas clouds and even stars, as it heats up and falls into the galaxy’s supermassive central black hole. But an open question in the physics of active galaxies is precisely how matter crosses the final few hundreds of light-years to reach the immediate neighborhood of the black hole before being swallowed.
“A study of this scope has become possible only recently, as the large surveys undertaken using the Hubble Space Telescope have become available,” said Mauricio Cisternas from the Max Planck Institute in Germany. “These have given us a huge sample of galaxies, both active and inactive, meaning that we can now study many distant galaxies in exquisite detail. Before these surveys, we hadn’t examined many active galaxies at large cosmic distances in sufficient detail.”
Cisternas and his team chose 140 active galaxies from the COSMOS survey. The COSMOS field is an area of sky roughly ten times the area covered by the Moon in the constellation Sextans the Sextant that has been comprehensively mapped by Hubble and other telescopes at different wavelengths. It contains several hundred thousand distant galaxies of all types. The team was able to identify active galaxies from among these using X-ray observations from the European Space Agency’s (ESA) XMM-Newton space telescope. They then studied the more detailed optical images of them taken by the NASA/ESA Hubble Space Telescope.
For each of the active galaxies in the study, they selected nine non-active galaxies at roughly the same distances and roughly in the same stage of cosmic evolution from the same Hubble images. This gives a total of just over 1,400 galaxies that the team could then test for the telltale signs of mergers.
“You can usually tell when galaxies have been involved in a merger,” said Knud Jahnke from the Max Planck Institute in Germany. “Instead of the neat, geometric spiral or smooth elliptical shapes you usually see in Hubble images, colliding galaxies typically look distorted and warped. We planned to find out whether these misshapen galaxies were more likely than regular ones to host active nuclei.”
Identifying whether or not a galaxy is distorted is a matter of judgment for which the expert eye of a trained astronomer is far better than any computerized assessment. To harness this human expertise without introducing the risk of unwitting bias, Cisternas set up a kind of identity parade of galaxies in which he had modeled and removed the bright spot that reveals the AGN. Ten galaxy experts, based at eight different institutions, independently assessed whether each of the galaxies was distorted or not, without being told which had an AGN.
None of the experts found a significant correlation between a galaxy’s activity and its distortion — that is between its black hole being well fed and its involvement in a major merger.
While mergers are a common phenomenon and are thought to play a role at least for some AGN, the study shows that they provide neither a universal nor a dominant mechanism for feeding black holes. By the study’s statistics, at least 75%, and possibly all, of AGN activity over the last 8 billion years must have a different explanation. Possible ways of transporting matter toward a central black hole include instabilities of structures like a spiral galaxy’s bar, the collisions of giant molecular clouds within the galaxy, or the fly-by of another galaxy that does not lead to a merger — known as galactic harassment.
Could there still be a causal connection between mergers and activity in the more distant past? That is the next question the group is gearing up to address. Suitable data is bound to come from two ongoing observational programs — Multi-Cycle Treasury Programs — with the Hubble Space Telescope as well as from observations by its successor, the James Webb Space Telescope, which is scheduled for launch after 2014.
Most galaxies, including our own, have a huge but well-behaved black hole at their heart, while some have messy eaters that suck in vast amounts of matter that then shines brightly as it falls towards oblivion. This causes the telltale bright spots at the center of galaxies known as active galactic nuclei (AGN). Why are the two types so different? Until now, the leading theory has been that mergers between galaxies are instrumental in driving matter into the black holes, making them grow.
In a new study, the largest of its kind so far, astronomers set up an identity parade of galaxies to test this theory. Comparing 140 active galaxies with a control group of over 1,200 comparable inactive galaxies, they found that there has been no significant link between AGN activity and galactic mergers for at least the past 8 billion years. Therefore, other phenomena, such as instabilities within galaxies, collisions of molecular clouds, or tidal disruption by other galaxies flying by, must be to blame.
The emission of radiation from AGNs is driven by the behavior of matter, such as gas clouds and even stars, as it heats up and falls into the galaxy’s supermassive central black hole. But an open question in the physics of active galaxies is precisely how matter crosses the final few hundreds of light-years to reach the immediate neighborhood of the black hole before being swallowed.
“A study of this scope has become possible only recently, as the large surveys undertaken using the Hubble Space Telescope have become available,” said Mauricio Cisternas from the Max Planck Institute in Germany. “These have given us a huge sample of galaxies, both active and inactive, meaning that we can now study many distant galaxies in exquisite detail. Before these surveys, we hadn’t examined many active galaxies at large cosmic distances in sufficient detail.”
Cisternas and his team chose 140 active galaxies from the COSMOS survey. The COSMOS field is an area of sky roughly ten times the area covered by the Moon in the constellation Sextans the Sextant that has been comprehensively mapped by Hubble and other telescopes at different wavelengths. It contains several hundred thousand distant galaxies of all types. The team was able to identify active galaxies from among these using X-ray observations from the European Space Agency’s (ESA) XMM-Newton space telescope. They then studied the more detailed optical images of them taken by the NASA/ESA Hubble Space Telescope.
For each of the active galaxies in the study, they selected nine non-active galaxies at roughly the same distances and roughly in the same stage of cosmic evolution from the same Hubble images. This gives a total of just over 1,400 galaxies that the team could then test for the telltale signs of mergers.
“You can usually tell when galaxies have been involved in a merger,” said Knud Jahnke from the Max Planck Institute in Germany. “Instead of the neat, geometric spiral or smooth elliptical shapes you usually see in Hubble images, colliding galaxies typically look distorted and warped. We planned to find out whether these misshapen galaxies were more likely than regular ones to host active nuclei.”
Identifying whether or not a galaxy is distorted is a matter of judgment for which the expert eye of a trained astronomer is far better than any computerized assessment. To harness this human expertise without introducing the risk of unwitting bias, Cisternas set up a kind of identity parade of galaxies in which he had modeled and removed the bright spot that reveals the AGN. Ten galaxy experts, based at eight different institutions, independently assessed whether each of the galaxies was distorted or not, without being told which had an AGN.
None of the experts found a significant correlation between a galaxy’s activity and its distortion — that is between its black hole being well fed and its involvement in a major merger.
While mergers are a common phenomenon and are thought to play a role at least for some AGN, the study shows that they provide neither a universal nor a dominant mechanism for feeding black holes. By the study’s statistics, at least 75%, and possibly all, of AGN activity over the last 8 billion years must have a different explanation. Possible ways of transporting matter toward a central black hole include instabilities of structures like a spiral galaxy’s bar, the collisions of giant molecular clouds within the galaxy, or the fly-by of another galaxy that does not lead to a merger — known as galactic harassment.
Could there still be a causal connection between mergers and activity in the more distant past? That is the next question the group is gearing up to address. Suitable data is bound to come from two ongoing observational programs — Multi-Cycle Treasury Programs — with the Hubble Space Telescope as well as from observations by its successor, the James Webb Space Telescope, which is scheduled for launch after 2014.
