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.
Organisations
Publications
Jiménez-Serra I
(2011)
VARIABILITY OF THE SiO THERMAL LINE EMISSION TOWARD THE YOUNG L1448-mm OUTFLOW
in The Astrophysical Journal
Schnee S
(2010)
THE DUST EMISSIVITY SPECTRAL INDEX IN THE STARLESS CORE TMC-1C
in The Astrophysical Journal
Cazaux S
(2011)
INTERSTELLAR ICES AS WITNESSES OF STAR FORMATION: SELECTIVE DEUTERATION OF WATER AND ORGANIC MOLECULES UNVEILED
in The Astrophysical Journal
Viti S
(2011)
L1157-B1: WATER AND AMMONIA AS DIAGNOSTICS OF SHOCK TEMPERATURE
in The Astrophysical Journal
Corcoran M
(2010)
RECENT X-RAY VARIABILITY OF ? CARINAE: THE QUICK ROAD TO RECOVERY
in The Astrophysical Journal
Hernandez A
(2012)
A VIRIALIZED FILAMENTARY INFRARED DARK CLOUD
in The Astrophysical Journal
Hernandez A
(2011)
MAPPING LARGE-SCALE CO DEPLETION IN A FILAMENTARY INFRARED DARK CLOUD
in The Astrophysical Journal
Caselli P
(2012)
FIRST DETECTION OF WATER VAPOR IN A PRE-STELLAR CORE
in The Astrophysical Journal
Wagner A
(2009)
A COSMIC-RAY PRECURSOR MODEL FOR A BALMER-DOMINATED SHOCK IN TYCHO'S SUPERNOVA REMNANT
in The Astrophysical Journal
Caselli P
(2012)
Our astrochemical heritage
in The Astronomy and Astrophysics Review
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 |