High Energy Astrophysics at Southampton

Lead Research Organisation: University of Southampton
Department Name: Sch of Physics and Astronomy

Abstract

On the smallest scales we are interested in why pulsars seem to favour the low neutral hydrogen environments in the SMC. We are also interested in the products of stellar collisions and near misses in the high density environment of globular clusters, and in studying the compact objects (ie black holes, neutron stars, or white dwarfs) in our Galaxy which are strong emitter of optical light from hydgrogen atoms. Some galactic X-ray binary sources, which consist of black hole of similar mass to our sun together with a more normal star have, as well as accretion discs, through which matter spirals onto the black hole, strong jets. We want to understand the relationship between the emission from jets and from the hot X-ray emitting coronae and to find out how the jet might emerge from the corona. In some cases the disappearance of the inner disc is followed by ejection of material along the jet and we shall determine whether such behaviour is typical in Active Galaxies, ie galaxies whose emission is powered material falling onto (ie being accreted) by a massive black hole. In the 20-100 keV band where absorption of photons by cold gas is unimportant, and so we obtain a very clear view, we are surveying the Galactic Plane with INTEGRAL to determine an unbiased census of compact objects. As time goes on, we will extend that survey to the extragalactic sky. We study the X-ray variability of Active Galaxies to determine how they relate to galactic X-ray binaries sources and whether characteristic timescales reflect only mass or another parameter such as accretion rate. We are interested in the binary populations of nearby galaxies and in the so-called `ultra luminous X-ray sources (ULXs)'. ULXs may be the long sought after black holes with masses intermediate between those of galactic binaries and Active Galaxies and so are very important for testing mass-based scaling relationships. We are interested in how the emission in different wavebands (Gamma-ray, X-ray, optical/IR, radio) in binaries and Active Galaxies is related and what is the dependence on mass. We are interested how the jet emission from Active Galaxies heats clusters of galaxies. On the largest scales, we are interested in whether the different faint source populations which we see in the radio, X-ray and IR bands are just different manifestations of the same underlying phenomenon and how massive black hole growth might be related to growth of the galaxy in which the black hole lives. We are also building detailed theoretical models, using computers, to explain the complicated variability which we see in the sky at high energies.

Publications

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Arvalo P (2008) X-ray variability of the Seyfert 1 Markarian 335: power spectrum and time lags in Monthly Notices of the Royal Astronomical Society

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Page M (2006) X-ray spectra of sources in the 13HXMM-Newton/Chandra deep field in Monthly Notices of the Royal Astronomical Society

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Campana R (2008) X-ray observations of the Large Magellanic Cloud pulsar PSR B0540-69 and its pulsar wind nebula in Monthly Notices of the Royal Astronomical Society

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McGowan K (2007) X-ray bright sources in the Chandra Small Magellanic Cloud Wing Survey - detection of two new pulsars in Monthly Notices of the Royal Astronomical Society

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Peacock M (2009) Wide Field CAMera survey of M31 globular clusters: low-mass X-ray binaries in Monthly Notices of the Royal Astronomical Society: Letters

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Worrall D (2008) Where Centaurus A Gets Its X-Ray Knottiness in The Astrophysical Journal

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Dieball A (2007) Unveiling the Core of the Globular Cluster M15 in the Ultraviolet in The Astrophysical Journal

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Sguera V (2006) Unveiling Supergiant Fast X-Ray Transient Sources with INTEGRAL in The Astrophysical Journal

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Gänsicke B (2006) Ultraviolet Studies of Interacting Binaries in Astrophysics and Space Science

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Gäansicke B (2006) Ultraviolet Studies Of Interacting Binaries in Astrophysics and Space Science

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Summons D (2007) Timing evidence in determining the accretion state of the Seyfert galaxy NGC 3783 in Monthly Notices of the Royal Astronomical Society

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Hardcastle M (2006) The X-ray nuclei of intermediate-redshift radio sources X-ray nuclei of radio sources in Monthly Notices of the Royal Astronomical Society

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Detmers R (2008) The warm absorber in NGC 5548 The lean years in Astronomy & Astrophysics

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Niemela V (2008) The very massive X-ray bright binary system Wack 2134 (= WR 21a) ? in Monthly Notices of the Royal Astronomical Society

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Fender R (2007) The variable radio counterpart and possible large-scale jet of the new Z source XTE J1701-462 in Monthly Notices of the Royal Astronomical Society: Letters

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Körding E (2007) The variability plane of accreting compact objects The variability plane in Monthly Notices of the Royal Astronomical Society

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Lucas P (2008) The UKIDSS Galactic Plane Survey in Monthly Notices of the Royal Astronomical Society

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Bird A (2007) The Third IBIS/ISGRI Soft Gamma-Ray Survey Catalog in The Astrophysical Journal Supplement Series

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Seymour N (2008) The star formation history of the Universe as revealed by deep radio observations in Monthly Notices of the Royal Astronomical Society

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Witham A (2006) The properties of cataclysmic variables in photometric Ha surveys Properties of CVs in Ha surveys in Monthly Notices of the Royal Astronomical Society

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Soldi S (2008) The multiwavelength variability of 3C 273 in Astronomy & Astrophysics

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Tudose V (2006) The large-scale jet-powered radio nebula of Circinus X-1 in Monthly Notices of the Royal Astronomical Society

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Russell D (2007) The jet-powered optical nebula of Cygnus X-1 in Monthly Notices of the Royal Astronomical Society

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Witham A (2008) The IPHAS catalogue of Ha emission-line sources in the northern Galactic plane in Monthly Notices of the Royal Astronomical Society

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Knigge C (2008) The intrinsic fraction of broad-absorption line quasars in Monthly Notices of the Royal Astronomical Society