Merging galaxies break radio silence. Large Hubble survey confirms link between mergers and supermassive black holes with relativistic jets

Merging galaxies break radio silence.

Large Hubble survey confirms link between mergers and supermassive black holes with relativistic jets

In the most extensive survey of its kind ever conducted, a team of scientists have found an unambiguous link between the presence of supermassive black holes that power high-speed, radio-signal-emitting jets and the merger history of their host galaxies. Almost all of the galaxies hosting these jets were found to be merging with another galaxy, or to have done so recently. The results lend significant weight to the case for jets being the result of merging black holes and will be presented in the Astrophysical Journal.

A team of astronomers using the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 (WFC3) have conducted a large survey to investigate the relationship between galaxies that have undergone mergers and the activity of the supermassive black holes at their cores.

The team studied a large selection of galaxies with extremely luminous centres — known as active galactic nuclei (AGNs) — thought to be the result of large quantities of heated matter circling around and being consumed by a supermassive black hole. Whilst most galaxies are thought to host a supermassive black hole, only a small percentage of them are this luminous and fewer still go one step further and form what are known as relativistic jets [1]. The two high-speed jets of plasma move almost with the speed of light and stream out in opposite directions at right angles to the disc of matter surrounding the black hole, extending thousands of light-years into space. The hot material within the jets is also the origin of radio waves.

It is these jets that Marco Chiaberge from the Space Telescope Science Institute, USA (also affiliated with Johns Hopkins University, USA and INAF-IRA, Italy) and his team hoped to confirm were the result of galactic mergers [2].

The team inspected five categories of galaxies for visible signs of recent or ongoing mergers — two types of galaxies with jets, two types of galaxies that had luminous cores but no jets, and a set of regular inactive galaxies [3].

“The galaxies that host these relativistic jets give out large amounts of radiation at radio wavelengths,” explains Marco. “By using Hubble’s WFC3 camera we found that almost all of the galaxies with large amounts of radio emission, implying the presence of jets, were associated with mergers. However, it was not only the galaxies containing jets that showed evidence of mergers!” [4].

“We found that most merger events in themselves do not actually result in the creation of AGNs with powerful radio emission,” added co-author Roberto Gilli from Osservatorio Astronomico di Bologna, Italy. “About 40% of the other galaxies we looked at had also experienced a merger and yet had failed to produce the spectacular radio emissions and jets of their counterparts.”

Although it is now clear that a galactic merger is almost certainly necessary for a galaxy to host a supermassive black hole with relativistic jets, the team deduce that there must be additional conditions which need to be met. They speculate that the collision of one galaxy with another produces a supermassive black hole with jets when the central black hole is spinning faster — possibly as a result of meeting another black hole of a similar mass — as the excess energy extracted from the black hole’s rotation would power the jets.

“There are two ways in which mergers are likely to affect the central black hole. The first would be an increase in the amount of gas being driven towards the galaxy’s centre, adding mass to both the black hole and the disc of matter around it,” explains Colin Norman, co-author of the paper. “But this process should affect black holes in all merging galaxies, and yet not all merging galaxies with black holes end up with jets, so it is not enough to explain how these jets come about. The other possibility is that a merger between two massive galaxies causes two black holes of a similar mass to also merge. It could be that a particular breed of merger between two black holes produces a single spinning supermassive black hole, accounting for the production of jets.”

Future observations using both Hubble and the Atacama Large Millimeter/submillimeter Array (ALMA) are needed to expand the survey set even further and continue to shed light on these complex and powerful processes.
Notes

[1] Relativistic jets travel at close to the speed of light, making them one of the fastest astronomical objects known.

[2] The new observations used in this research were taken in collaboration with the 3CR-HST team. This international team of astronomers is currently led by Marco Chiaberge and has conducted a series of surveys of radio galaxies and quasars from the 3CR catalogue using the Hubble Space Telescope.

[3] The team compared their observations with the swathes of archival data from Hubble. They directly surveyed twelve very distant radio galaxies and compared the results with data from a large number of galaxies observed during other observing programmes.

[4] Other studies had shown a strong relationship between the merger history of a galaxy and the high levels of radiation at radio wavelengths that suggests the presence of relativistic jets lurking at the galaxy’s centre. However, this survey is much more extensive, and the results very clear, meaning it can now be said with almost certainty that radio-loud AGNs, that is, galaxies with relativistic jets, are the result of galactic mergers.

Artist’s illustration of galaxy with jets from a supermassive black hole

This artist’s impression illustrates how high-speed jets from supermassive black holes would look. These outflows of plasma are the result of the extraction of energy from a supermassive black hole’s rotation as it consumes the disc of swirling material that surrounds it. These jets have very strong emissions at radio wavelengths.

Credit:

ESA/Hubble, L. Calçada (ESO)

Galaxies with relativistic jets

This image taken with the NASA/ESA Hubble Space Telescope shows a selection of galaxies used in a survey to confirm the link between mergers and high-speed jets from supermassive black holes. These galaxies have very strong emissions at radio wavelengths, implying that the supermassive black holes they host are feeding huge outflows of plasma.

On the left (top to bottom) are the galaxies 3C 297 and 3C 454.1, on the right is 3C 356.

Credit:

NASA, ESA, M. Chiaberge (STScI)

Radio galaxy 3C 297

This image taken with the NASA/ESA Hubble Space Telescope shows the galaxy 3C 297, which was part of a large survey of galaxies.

The survey confirmed the link between mergers and galaxies hosting relativistic jets from supermassive black holes. These galaxies have very strong emissions at radio wavelengths implying that the supermassive black holes they host are feeding huge outflows of plasma.

Credit:

NASA, ESA, M. Chiaberge (STScI)

Radio galaxy 3C 454.1

This image taken with the NASA/ESA Hubble Space Telescope shows the galaxy 3C 454.1 which was part of a large survey of galaxies.

The survey confirmed the link between mergers and galaxies hosting jets travelling near the speed of light from supermassive black holes. These galaxies have very strong emissions at radio wavelengths implying that the supermassive black holes they host are feeding huge outflows of plasma.

Credit:

NASA, ESA, M. Chiaberge (STScI)

Radio galaxy 3C 356

This image taken with the NASA/ESA Hubble Space Telescope shows the galaxy 3C 356 which was part of a large survey of galaxies.
The survey confirmed the link between mergers and galaxies hosting relativistic jets from supermassive black holes. These galaxies have very strong emissions at radio wavelengths implying that the supermassive black holes they host are feeding huge outflows of plasma.

Credit:

NASA, ESA, M. Chiaberge (STScI)

VIDEOS .

Artist’s animation of galaxy with jets from a supermassive black hole

http://www.spacetelescope.org/videos/heic1511a/

This artist’s impression illustrates how high-speed jets from supermassive black holes would look. These outflows of plasma are the result of the extraction of energy from a supermassive black hole’s rotation as it consumes the disc of swirling material that surrounds it. These jets have very strong emissions at radio wavelengths.

Credit:

ESA/Hubble, L. Calçada (ESO)

Fulldome clip showing animation of galaxy with jets from a supermassive black hole

http://www.spacetelescope.org/videos/heic1511b/

This artist’s impression illustrates how high-speed jets from supermassive black holes would look. These outflows of plasma are the result of the extraction of energy from a supermassive black hole’s rotation as it consumes the disc of swirling material that surrounds it. These jets have very strong emissions at radio wavelengths.

Credit:

ESA/Hubble, L. Calçada (ESO)

Fuente: ESA/Hubble Information Centre