9th January 2017 - Monster black holes sometimes play a cosmic game of hide and seek, shrouding themselves from view behind giant clouds of gas and dust, according to new research.
Scientists believe supermassive black holes lurk at the centres of most big galaxies, but many are hidden from the view of most telescopes.
Now astronomers at the universities of Durham and Southampton, working with NASA’s Jet Propulsion Laboratory (JPL), have confirmed in separate studies that two of these cosmic giants had been hidden by thick layers of gas and dust at the heart of galaxies near to our own Milky Way.
NGC 1448, a galaxy with an active galactic nucleus hidden by gas and dust, is seen in this image
(Credit: : Carnegie-Irvine Galaxy Survey/NASA/JPL-Caltech)
Using NASA’s space-based NuSTAR (Nuclear Spectroscopic Telescope Array) mission, the scientists were able to detect high-energy X-ray emissions generated by the black holes as they feed on surrounding material.
The research could provide more information about supermassive black holes, allowing them to be studied in more detail.
The Durham team was co-funded by STFC. Ady Annuar, a postgraduate researcher in the Department of Physics, Durham University, led a study looking at the black hole at the centre of the NGC 1448 spiral galaxy.
NGC 1448 is one of the nearest large galaxies to our Milky Way at 38 million light years away (one light year is about six trillion miles).
The study found that the galaxy had a thick column of gas at the nucleus, hiding the central black hole that was only discovered in 2009.
X-ray emissions as seen by NuSTAR and the Chandra X-ray Observatory suggest for the first time that there must be a thick layer of gas and dust shielding the active black hole in the galaxy from view.
Ady Annuar, who is also a member of Durham University’s Centre for Extragalactic Astronomy, said: "These black holes are relatively close to the Milky Way, but they have remained hidden from us until now.
"They're like monsters hiding under your bed.”
Research co-author Professor David Alexander, in the Department of Physics, at Durham University, added: “These hidden monsters have been predicted to be fairly abundant in our Universe.
“It is only after the advent of NuSTAR that we actually began to find each of them one by one.”
The Durham-led study also found that NGC 1448 has a large population of young (five-million-year-old) stars, suggesting that the galaxy produces new stars at the same time that its black hole feeds on gas and dust.
In a similar study, researchers led by the University of Southampton, looked at an active galaxy called IC 3639, which is 170 million light years away.
Researchers analysed data from this object alongside previous observations from Chandra and the Japanese-led Suzaku satellite.
As with the NGC 1448 galaxy, they confirmed the nature of IC 3639 as an active galactic nucleus – a class of extremely bright objects that includes quasars and blazars.
NuSTAR also provided the first precise measurement of how much material is obscuring the central engine of IC 3639, allowing researchers to determine how luminous this hidden monster really is.
STFC Press Officer
Notes to Editors
Active galactic nuclei are so bright because particles in the regions around the black hole get very hot and emit radiation. However, most active nuclei are believed to be surrounded by a doughnut-shaped region of thick gas and dust that obscures the central regions from certain lines of sight.
Both of the active galactic nuclei that NuSTAR recently studied appear to be oriented so that astronomers view them edge-on. That means that instead of seeing the bright central regions, telescopes primarily see the reflected X-rays from the doughnut-shaped obscuring material.
NuSTAR is a Small Explorer mission led by Caltech and managed by JPL for NASA's Science Mission Directorate in Washington. NuSTAR was developed in partnership with the Danish Technical University and the Italian Space Agency (ASI). The spacecraft was built by Orbital Sciences Corp., Dulles, Virginia. NuSTAR's mission operations center is at UC Berkeley, and the official data archive is at NASA's High Energy Astrophysics Science Archive Research Center. ASI provides the mission's ground station and a mirror archive. JPL is managed by Caltech for NASA.
The Durham University study was funded by Majlis Amanah Rakyat (MARA) Malaysia and the Science and Technology Facilities Council.
NGC 1448, a galaxy with an active galactic nucleus hidden by gas and dust, is seen in this image.
Credit: Carnegie-Irvine Galaxy Survey/NASA/JPL-Caltech
Department of Physics, Durham University: www.durham.ac.uk/physics/
Centre for Extragalactic Astronomy: http://astro.dur.ac.uk/Cosmology/
NuSTAR: www.nasa.gov/nustar; www.nustar.caltech.edu/