Black holes and galaxy death
16-Apr-2010, Plain html version.
Royal Astronomical Society Press Release
RAS PN 10/37 (NAM 22)
April 9th 2010
Black holes and galaxy death
Black holes are thought to reside at the centre of almost every galaxy, with some growing to more than a billion times the mass of the Sun. Now a team of UK astronomers believe that these supermassive black holes are commonplace, release more than enough energy to strip their host galaxies apart and in the process shut down these galaxies' star formation for good. On Friday 16th April, team member Asa Bluck of the University of Nottingham, who led this research, will explain the dramatic impact of these monster black holes in his talk at the RAS National Astronomy Meeting (NAM 2010) in Glasgow.
For many years black holes have fascinated scientists and the public alike, with their peculiar ability to warp space and time and their almost sinister tendency to devour everything they encounter. Before it falls in, as matter swirls around the black hole it forms an "accretion disk", where it heats up and radiates energy. The supermassive black holes have such a strong gravitational field that the infalling matter releases a vast amount of energy, making each accretion disk far brighter than the combined output of the hundreds of billions of stars in the galaxy around it.
One of the consequences of this outpouring of energy is that it drives away cool gas and dust, the raw ingredients of new stars. This permanently shuts down star formation in the surrounding galaxy, dooming it to a slow death, where the remaining stars age, grow red, end their lives and are never replaced.
The new study considered the role of supermassive black holes in the development of galaxies. To search for them, the team used the Hubble Space Telescope and the Chandra X-ray Observatory to image the Universe to unprecedented depth and resolution in optical, near infra-red and X-ray light. In particular, the astronomers looked for galaxies which have a very high emission of X-rays, a classic signature of black holes devouring gas and dust.
From the space telescopes' data Asa and the other team members find that at least 1/3 of all the massive galaxies in the Universe not only contain supermassive black holes, but that at some point in their histories the emission from the holes' accretion disks far outshines their host galaxies. The energy output of regions around the black holes is high enough to strip apart every massive galaxy in the cosmos 25 times over, whilst the X-ray emission from them turns out to dwarf that from every other source in the Universe put together.
Asa sums up the new results: "We are left with a startling picture of the formation history of massive galaxies, where dramatic violence in the form of the torrent of radiation from matter falling into black holes leads to the death of galaxies they inhabit."
University of Nottingham
NAM 2010 Press Office (12th - 16th April only)
Gilbert Scott Building
University of Glasgow
Tel: +44 (0)141 330 7409, +44 (0)141 330 7410, +44 (0)141 330 7411
Dr Robert Massey
Press and Policy Officer
Royal Astronomical Society
Mob: +44 (0)794 124 8035
Royal Astronomical Society
Mob: +44 (0)7756 034 243
Image Caption: The image is a multi-wavelength image of the galaxy NGC 1275 which is a local equivalent to many of the distant massive galaxies studied by Asa Bluck and the other members of the Nottingham / University College London team. It shows the phenomenal power of supermassive Black Holes to rearrange the gas of a galaxy, and represents a window onto a violent past to the lives of galaxies. Over the history of the Universe at least 1/3 of all galaxies went through a phase of development similar to this one. Credit: A. Fabian (Cambridge) / STScI / NASA. Full Size version.
The results of this study are to be submitted to Monthly Notices of the Royal Astronomical Society for publication.
NOTES FOR EDITORS
RAS NATIONAL ASTRONOMY MEETING (NAM 2010)
The RAS National Astronomy Meeting 2010 will take place from 12-16th April at the University of Glasgow. The conference is held in conjunction with the UK Solar Physics (UKSP) and Magnetosphere Ionosphere and Solar-Terrestrial Physics (MIST) meetings. NAM2010 (www.astro.gla.ac.uk/nam2010/) is principally sponsored by the Royal Astronomical Society (RAS) and the University of Glasgow.
THE ROYAL ASTRONOMICAL SOCIETY
The Royal Astronomical Society (RAS: www.ras.org.uk), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organises scientific meetings, publishes international research and review journals, recognises outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.
THE UNIVERSITY OF GLASGOW
The University of Glasgow (founded 1451) is one of the world’s top 100 research universities with more than 70 per cent of its research rated as world-leading or internationally excellent. The Physics and Astronomy Department is one of the top four in the UK’s major research-intensive universities, the Russell Group.
The conference comes to Glasgow during the 250th anniversary year of the founding of the Regius Chair of Astronomy at the University of Glasgow, first held by astronomer and meteorologist Alexander Wilson in 1760. The present incumbent is Prof. John Brown, 10th Astronomer Royal for Scotland.