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

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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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Goldsmith P (2011) HERSCHEL MEASUREMENTS OF MOLECULAR OXYGEN IN ORION in The Astrophysical Journal

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Green J (2009) The 6-GHz multibeam maser survey - I. Techniques in Monthly Notices of the Royal Astronomical Society

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Havnes O (2011) In-flight calibration of mesospheric rocket plasma probes. in The Review of scientific instruments

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Hernandez A (2012) A VIRIALIZED FILAMENTARY INFRARED DARK CLOUD in The Astrophysical Journal

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Hernandez A (2011) MAPPING LARGE-SCALE CO DEPLETION IN A FILAMENTARY INFRARED DARK CLOUD in The Astrophysical Journal

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Hily-Blant P (2010) Nitrogen hydrides in the cold envelope of IRAS 16293-2422 in Astronomy and Astrophysics

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Hoare M (2012) The Coordinated Radio and Infrared Survey for High-Mass Star Formation (The CORNISH Survey). I. Survey Design in Publications of the Astronomical Society of the Pacific

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Jiang Zhibo (2008) Disks around massive young stellar objects: Are they common? in ASTROPHYSICAL JOURNAL LETTERS

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Jiménez-Serra I (2010) Parsec-scale SiO emission in an infrared dark cloud Parsec-scale SiO emission in an IRDC in Monthly Notices of the Royal Astronomical Society

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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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Jiménez-Serra I (2008) Parametrization of C-shocks. Evolution of the sputtering of grains in Astronomy & 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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Keto E (2010) Dynamics and depletion in thermally supercritical starless cores in Monthly Notices of the Royal Astronomical Society

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Keto Eric (2008) The different structures of the two classes of starless cores in ASTROPHYSICAL JOURNAL

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Komissarov S (2012) Shock dissipation in magnetically dominated impulsive flows Shock dissipation in Monthly Notices of the Royal Astronomical Society

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Komissarov S (2011) 3+1 magnetodynamics in Monthly Notices of the Royal Astronomical Society: Letters

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Komissarov S (2009) Magnetic acceleration of ultrarelativistic jets in gamma-ray burst sources in Monthly Notices of the Royal Astronomical Society

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Komissarov S (2011) On the origin of variable gamma-ray emission from the Crab nebula Gamma-ray emission from the Crab nebula in Monthly Notices of the Royal Astronomical Society

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Komissarov S (2009) Activation of the Blandford-Znajek mechanism in collapsing stars in Monthly Notices of the Royal Astronomical Society

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Komissarov S (2010) Supercollapsars and their X-ray bursts in Monthly Notices of the Royal Astronomical Society: Letters

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Komissarov Serguei S. (2009) Blandford-Znajek Mechanism versus Penrose Process in JOURNAL OF THE KOREAN PHYSICAL SOCIETY

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Lis D (2010) Herschel /HIFI discovery of interstellar chloronium (H 2 Cl + ) in Astronomy and Astrophysics

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

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

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Maiolino R (2009) Strong [CII] emission at high redshift 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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Mendigutía I (2012) Accretion-related properties of Herbig Ae/Be stars Comparison with T Tauris? in Astronomy & Astrophysics

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