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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Liseau R (2012) Multi-line detection of O 2 toward ? Ophiuchi A in Astronomy & Astrophysics

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Fontani F (2011) Deuteration as an evolutionary tracer in massive-star formation in Astronomy & Astrophysics

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

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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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De Wit W (2008) Resolved 24.5 micron emission from massive young stellar objects in Astronomy & Astrophysics

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Oudmaijer R (2008) Sub-milliarcsecond precision spectro-astrometry of Be stars in Astronomy & Astrophysics

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Maiolino R (2009) Strong [CII] emission at high redshift in Astronomy & Astrophysics

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Vink J (2009) On the presence and absence of disks around O-type stars in Astronomy & Astrophysics

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Jiménez-Serra I (2008) Parametrization of C-shocks. Evolution of the sputtering of grains in Astronomy & 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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Gallerani S (2012) Resolved [CII] emission in a lensed quasar at z = 4.4 in Astronomy & Astrophysics

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Mendigutía I (2011) Optical spectroscopic variability of Herbig Ae/Be stars in Astronomy & Astrophysics

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Wheelwright H (2009) The close Be star companion of $\mathrm \beta$ Cephei in Astronomy & Astrophysics

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De Breuck C (2011) Enhanced [CII] emission in a z = 4.76 submillimetre galaxy in Astronomy & 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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Mendigutía I (2012) Accretion-related properties of Herbig Ae/Be stars Comparison with T Tauris? in Astronomy & Astrophysics

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Nagao T (2012) ALMA reveals a chemically evolved submillimeter galaxy at z = 4.76 in Astronomy & Astrophysics

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Mendigutía I (2011) Accretion rates and accretion tracers of Herbig Ae/Be stars in Astronomy & Astrophysics

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Van Loo S (2012) Magnetic fields and star formation in Astronomy & Geophysics

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

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Bacmann A (2010) First detection of ND in the solar-mass protostar IRAS16293-2422 in Astronomy and 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