A rolling grant for the observation and study of cosmic X-ray sources (Apr 2009 to Mar 2014)
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
The X-ray Group at the Institute of Astronomy has analysed and interpreted data from most cosmic X-ray telescopes and instruments. This grant application is to renew the rolling grant for its support. Over the next five years we shall pursue a programme of research centred on accreting black holes and clusters of galaxies. The most luminous non-explosive sources in the Universe are active galaxies and quasars, which are powered by an accreting black hole. Most of the X-ray emission from these objects originates close to the black hole where gravity is very strong. This causes high velocities and large redshifts, both doppler and gravitational, as well as strong bending of light. The emission spectrum from matter at the innermost radii is consequently highly distorted in a manner first discovered by us and which is easily recognised. We propose to measure these relativistic distortion using both the X-ray spectrum and its variability. The results can then be used to determine the geometry of the accretion flow and the source of the X-ray continuum. Through the location of the innermost orbit, we shall measure the spin of the black hole. The energy produced by a central massive black hole can have a profound effect on its host galaxy. This can be vividly observed when the galaxy is at the centre of a group or cluster of galaxies and the energy is emitted through jets. X-ray images show bubbles filled with relativitic plasma inflating and rising through the surrounding gas. Concentric ripples show energy flowing away from the bubbles in giant sound waves discovered by us and which dissipate heating the surrounding gas. The energy transferred in this way stops much of the gas from cooling rapidly and forming massive amounts of new stars. Filaments of cold gas are dragged around by the bubbles so marking the velocity field of the cluster core. We shall analyse and interpret X-ray and longer wavelength observations of the cores of groups and clusters in order to understand this important galaxy feedback process, including how and when a heating/cooling balance is established, how much cooling and star formation takes place and how much it applies to the formation of all massive galaxies. Funding for Postdoctoral Research Assistants to work on these exciting and fundamental topics in astrophysics is sought for a five year programme.
Organisations
Publications
Edge A
(2010)
Herschel observations of FIR emission lines in brightest cluster galaxies
in Astronomy and Astrophysics
Ehlert S
(2011)
Extreme active galactic nucleus feedback and cool-core destruction in the X-ray luminous galaxy cluster MACS J1931.8-2634 Extreme feedback in MACS J1931.8-2634
in Monthly Notices of the Royal Astronomical Society
Fabian A
(2011)
A wide Chandra view of the core of the Perseus cluster A wider view of the Perseus cluster
in Monthly Notices of the Royal Astronomical Society
Fabian A
(2011)
The energy source of the filaments around the giant galaxy NGC 1275 Power to the filaments
in Monthly Notices of the Royal Astronomical Society
Fabian AC
(2009)
Broad line emission from iron K- and L-shell transitions in the active galaxy 1H 0707-495.
in Nature
Fridriksson J
(2011)
THE VARIABLE QUIESCENT X-RAY EMISSION OF THE TRANSIENT NEUTRON STAR XTE J1701-462
in The Astrophysical Journal
George M
(2009)
X-ray observations of the galaxy cluster PKS 0745-191: to the virial radius, and beyond
in Monthly Notices of the Royal Astronomical Society
Hamer S
(2012)
The relation between line emission and brightest cluster galaxies in three exceptional clusters: evidence for gas cooling from the intracluster medium Offset optical line emission in cluster cores
in Monthly Notices of the Royal Astronomical Society
Hlavacek-Larrondo J
(2012)
Extreme AGN feedback in the MAssive Cluster Survey: a detailed study of X-ray cavities at z>0.3 X-ray cavities in the MACS cluster sample
in Monthly Notices of the Royal Astronomical Society
Hlavacek-Larrondo J
(2011)
AGN feedback and iron enrichment in the powerful radio galaxy, 4C+55.16 The cluster around 4C+55.16
in Monthly Notices of the Royal Astronomical Society