A team of researchers, mainly from Centro de Astrofísica da Universidade do Porto (CAUP), has detected a rare type of active galactic nuclei (AGNs), which have simultaneously characteristics of young and old AGNs. This apparent discrepancy is thought to be due to a recent re-ignition of the central black hole.
Black and white image of the AGN in the maxBCG 2596 region, in the near infrared. Superimposed in red are the radio contours, with the lobes visible on either side
(Filho et al. 2011)
The team cross-correlated a catalogue of over 13 thousand clusters with a catalogue at radio frequencies, searching for a link between AGNs and the clusters in which they reside. CAUP astronomer and principal investigator, Mercedes Filho, commented on this chance discovery: “Our initial project aimed to study radio galaxies in clusters. By chance, we found eight radio sources with extended structure (radio jets and lobes) that didn’t show up in the optical images, which we found strange. So we decided to drop the initial project and pursue these strange radio galaxies”.
The team cross-correlated a catalogue of over 13 thousand clusters with a catalogue at radio frequencies, searching for a link between AGNs and the clusters in which they reside. CAUP astronomer and principal investigator, Mercedes Filho, commented on this chance discovery: “Our initial project aimed to study radio galaxies in clusters. By chance, we found eight radio sources with extended structure (radio jets and lobes) that didn’t show up in the optical images, which we found strange. So we decided to drop the initial project and pursue these strange radio galaxies”.
Artist's impression of an AGN with interrupted jets.
(original image credit: Aurore Simonnet, Sonoma State University)
In order to get more information about these eight objects, further observations in the infrared were made with the VLT (ESO). This allowed the team to detect the host galaxies, where the extended radio structures originated from.
While comparing the obtained spectra with known galaxy models, the team was able to conclude that these eight sources are rare objects – galaxies with characteristics common to active AGNs (that still have jet emission), and inactive AGNs (where the jet emission has turned off). This (apparent) discrepancy can be explained with a relatively recent reactivation of the AGN, due to new material being accreted by the central black hole.
In order to get more information about these eight objects, further observations in the infrared were made with the VLT (ESO). This allowed the team to detect the host galaxies, where the extended radio structures originated from.
While comparing the obtained spectra with known galaxy models, the team was able to conclude that these eight sources are rare objects – galaxies with characteristics common to active AGNs (that still have jet emission), and inactive AGNs (where the jet emission has turned off). This (apparent) discrepancy can be explained with a relatively recent reactivation of the AGN, due to new material being accreted by the central black hole.
Video still from a simulation of an AGN with intermittent jet emission (13 million year cycles), during a period of 192 million years.
(Peter Mendygral (Minnesota Supercomputing Institute)/Klaus Dolag/Tom Jones). Video available at: http://youtu.be/YpQkg5j_8sM?hd=1
In general, when a black hole is active, it produces a jet along the galaxy's rotation axis. This jet can travel great distances, creating lobes visible at radio frequencies. When the black hole is not active, the jet shuts down, but the lobes can persist for a very long time (a minimum of 1 million years).
The original jet emission must have been interrupted sometime in the past, while the lobes, though fading, remain visible in the radio. According to Mercedes Filho “our objects have radio lobes, a sign of past activity, but the spectra tells us that the central black hole and the jet have recently been reactivated”.
The black hole must have recently been replenished of new material (either through internal disk instabilities or interactions with other galaxies), which instigated a new jet emission, that started before the original radio lobes faded completely.
The team will now carry out a new set of observations, both in radio and gamma rays, to try and detect direct hints of young jets associated with the re-ignited central black hole.
Contacts and sources:
In general, when a black hole is active, it produces a jet along the galaxy's rotation axis. This jet can travel great distances, creating lobes visible at radio frequencies. When the black hole is not active, the jet shuts down, but the lobes can persist for a very long time (a minimum of 1 million years).
The original jet emission must have been interrupted sometime in the past, while the lobes, though fading, remain visible in the radio. According to Mercedes Filho “our objects have radio lobes, a sign of past activity, but the spectra tells us that the central black hole and the jet have recently been reactivated”.
The black hole must have recently been replenished of new material (either through internal disk instabilities or interactions with other galaxies), which instigated a new jet emission, that started before the original radio lobes faded completely.
The team will now carry out a new set of observations, both in radio and gamma rays, to try and detect direct hints of young jets associated with the re-ignited central black hole.
Contacts and sources:
Citation: Optically Faint Radio Sources: Reborn AGN?
A&A Volume 536, December 2011 (DOI: 10.1051/0004-6361/201117834)
A&A Volume 536, December 2011 (DOI: 10.1051/0004-6361/201117834)
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