A Rolling Programme of Astrophysical Research at Leeds

Lead Research Organisation: University of Leeds
Department Name: Applied Mathematics

Abstract

Many astrophysical phenomena involve a complicated interaction between physical and chemical processes and fluid dynamics. We intend to use a combination of analysis and novel numerical methods, based on adaptive grids, to investigate such phenomena, in particular those involved in star formation, interactions between stars and their environment, starburst galaxies and active galactic nuclei, pulsar wind nebulae and the magnetospheres of pulsars and black holes. The emphasis is on generic processes that are important in a wide range of astrophysical objects. The star formation theme will combine the theoretical work with molecular line observations, multi-wavelength surveys of our Galaxy and the latest high resolution observations of the circumstellar environment of massive stars.

Publications

10 25 50

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Parkin E (2011) X-RAY EMISSION FROM THE DOUBLE-BINARY OB-STAR SYSTEM QZ CAR (HD 93206) in The Astrophysical Journal Supplement Series

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Caselli P (2010) Water vapor toward starless cores: The Herschel view in Astronomy and Astrophysics

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Van Dishoeck E. F. (2011) Water in Star-forming Regions with the Herschel Space Observatory (WISH). I. Overview of Key Program and First Results in PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC

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Chavarría L (2010) Water in massive star-forming regions: HIFI observations of W3 IRS5 in Astronomy and Astrophysics

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Wheelwright H (2012) VLTI/AMBER observations of the binary B[e] supergiant HD 327083 in Astronomy & Astrophysics

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Wyrowski F (2010) Variations in H 2 O + /H 2 O ratios toward massive star-forming regions in Astronomy and Astrophysics

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Jiménez-Serra I (2011) VARIABILITY OF THE SiO THERMAL LINE EMISSION TOWARD THE YOUNG L1448-mm OUTFLOW in The Astrophysical Journal

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Jiménez-Serra I (2009) UNVEILING THE MAIN HEATING SOURCES IN THE CEPHEUS A HW2 REGION in The Astrophysical Journal

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Ashmore I (2010) Transient evolution of C-type shocks in dusty regions of varying density in Astronomy and Astrophysics

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Van Loo S (2009) Time-dependent simulations of steady C-type shocks 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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Pittard J (2010) The turbulent destruction of interstellar clouds in Astrophysics and Space Science

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Pittard J (2010) The turbulent destruction of clouds - II. Mach number dependence, mass-loss rates and tail formation in Monthly Notices of the Royal Astronomical Society

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Stead J (2009) The slope of the near-infrared extinction law in Monthly Notices of the Royal Astronomical Society

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Cazaux S (2008) The role of carbon grains in the deuteration of H 2 in Astronomy & Astrophysics

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Mottram J (2010) The RMS survey: far-infrared photometry of young massive stars in Astronomy and Astrophysics

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Emprechtinger M (2008) The N 2 D + /N 2 H + ratio as an evolutionary tracer of Class 0 protostars in Astronomy & Astrophysics

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Wheelwright H (2010) The mass ratio and formation mechanisms of Herbig Ae/Be star binary systems in Monthly Notices of the Royal Astronomical Society

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Pope E (2008) The generation of optical emission-line filaments in galaxy clusters in Monthly Notices of the Royal Astronomical Society

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Van Loo S (2008) The effect of ambipolar resistivity on the formation of dense cores in Astronomy & Astrophysics

 
Description Star formation occurs due to the collapse of interstellar clouds due to their own gravitational attraction. We have shown that the interstellar magnetic field plays an important role in forming the clouds that can collapse to form stars.
Exploitation Route It is now generally recognised that magnetic fields and in particular non-ideal effects such as ambi-polar diffusion play an important role in the formation of the clouds that collapse to form stars.
Sectors Aerospace, Defence and Marine,Energy,Environment

 
Description The observational work has improved our understanding of massive star formation. The theoretical work has shown that magnetic fields play a major role in the early stages of star formation.
First Year Of Impact 2010
Sector Aerospace, Defence and Marine,Energy,Environment
Impact Types Cultural,Economic

 
Description Star Formation and Protoplanetary Discs
Amount £1,546,225 (GBP)
Funding ID ST/I001557/1 
Organisation Science and Technologies Facilities Council (STFC) 
Sector Public
Country United Kingdom
Start 04/2011 
End 03/2014