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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Molinari S. (2010) Hi-GAL: The Herschel Infrared Galactic Plane Survey in PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC

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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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Caselli P (2012) Our astrochemical heritage in The Astronomy and Astrophysics Review

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Pineda J (2010) DIRECT OBSERVATION OF A SHARP TRANSITION TO COHERENCE IN DENSE CORES 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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Pillai T (2012) H 2 D + IN THE HIGH-MASS STAR-FORMING REGION CYGNUS X in The Astrophysical Journal

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

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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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Schnee S (2010) THE DUST EMISSIVITY SPECTRAL INDEX IN THE STARLESS CORE TMC-1C in The Astrophysical Journal

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Viti S (2011) L1157-B1: WATER AND AMMONIA AS DIAGNOSTICS OF SHOCK TEMPERATURE in The Astrophysical Journal

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Corcoran M (2010) RECENT X-RAY VARIABILITY OF ? CARINAE: THE QUICK ROAD TO RECOVERY in The Astrophysical Journal

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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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Caselli P (2012) FIRST DETECTION OF WATER VAPOR IN A PRE-STELLAR CORE in The Astrophysical Journal

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Townsley L (2011) THE CHANDRA CARINA COMPLEX PROJECT: DECIPHERING THE ENIGMA OF CARINA'S DIFFUSE X-RAY EMISSION in The Astrophysical Journal Supplement Series

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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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Nazé Y (2011) GLOBAL X-RAY PROPERTIES OF THE O AND B STARS IN CARINA in The Astrophysical Journal Supplement Series

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Townsley L (2011) AN INTRODUCTION TO THE CHANDRA CARINA COMPLEX PROJECT in The Astrophysical Journal Supplement Series

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

 
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