Astronomers find black hole is 30 times expected size
This one though is really too big for its boots – it simply shouldn’t be possible
for it to be so large”, Dr Jacco van Loon, Keele, lead author on the paper.
The central supermassive black hole of a recently discovered galaxy has been found to be far larger than should be possible, according to current theories of galactic evolution. New work, carried out by astronomers at Keele University and the University of Central Lancashire, shows that the black hole is much more massive than it should be, compared to the mass of the galaxy around it. The scientists publish their results in a paper in Monthly Notices of the Royal Astronomical Society.
The galaxy, SAGE0536AGN, was initially discovered with NASA's Spitzer Space Telescope in infrared light. Thought to be at least 9 billion years old, it contains an active galactic nucleus (AGN), an incredibly bright object resulting from the accretion of gas by a central supermassive black hole. The gas is accelerated to high velocities due to the black hole's immense gravitational field, causing this gas to emit light.
The team has now also confirmed the presence of the black hole by measuring the speed of the gas moving around it. Using the Southern African Large Telescope, the scientists observed that an emission line of hydrogen in the galaxy spectrum (where light is dispersed into its different colours – a similar effect is seen using a prism) is broadened through the Doppler Effect, where the wavelength (colour) of light from objects is blue- or red-shifted depending on whether they are moving towards or away from us.
The degree of broadening implies that the gas is moving around at high speed, a result of the strong gravitational field of the black hole.
These data have been used to calculate the black hole's mass: the more massive the black hole, the broader the emission line. The black hole in SAGE0536AGN was found to be 350 million times the mass of the Sun. But the mass of the galaxy itself, obtained through measurements of the movement of its stars, has been calculated to be 25 billion solar masses. This is seventy times larger than that of the black hole, but the black hole is still thirty times larger than expected for this size of galaxy.
“Galaxies have a vast mass, and so do the black holes in their cores. This one though is really too big for its boots – it simply shouldn’t be possible for it to be so large”, said Dr Jacco van Loon, an astrophysicist at Keele University and the lead author on the new paper.
In ordinary galaxies the black hole would grow at the same rate as the galaxy, but in SAGE0536AGN the black hole has grown much faster, or the galaxy stopped growing prematurely. Because this galaxy was found by accident, there may be more such objects waiting to be discovered. Time will tell whether SAGE0536AGN really is an oddball, or simply the first in a new class of galaxies.
Media contact
Dr Robert Massey
Royal Astronomical Society
Tel: +44 (0)20 7734 3307
Mob: +44 (0)7802 877 699
Science contact
Dr Jacco van Loon
Keele University
Tel: +44(0)1782 73 3331
Mob: +44(0)7791 805 260
Images and captions
https://www.ras.org.uk/images/stories/press/galaxies/SAGE0536AGN_VMC.jpg
An image of the galaxy SAGE0536AGN, from the Vista Magellanic Clouds survey.
The galaxy is the elliptical object in the centre of the frame.
https://www.ras.org.uk/images/stories/press/galaxies/NASA AGN illustration.jpg
A still frame from a movie, illustrating an active galactic nucleus, with jets of material flowing from out from a central black hole. Credit: NASA / Dana Berry / SkyWorks Digital (See http://www.nasa.gov/centers/goddard/mov/103893main_3SpeedyHotSpots.mov for the full movie.)
Further information
The new work appears in “An evolutionary missing link? A modest-mass early-type galaxy hosting an oversized nuclear black hole”, Jacco Th. van Loon and Anne E. Sansom, Monthly Notices of the Royal Astronomical Society, vol. 453 (3), pp. 2341-2348, Oxford University Press.
The paper can be downloaded from
http://mnras.oxfordjournals.org/content/453/3/2341
Notes for editors
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