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
Keto E
(2010)
Dynamics and depletion in thermally supercritical starless cores
in Monthly Notices of the Royal Astronomical Society
De Breuck C
(2011)
Enhanced [CII] emission in a z = 4.76 submillimetre galaxy
in Astronomy & Astrophysics
Codella C
(2012)
ERRATUM: "THE HERSCHEL AND IRAM CHESS SPECTRAL SURVEYS OF THE PROTOSTELLAR SHOCK L1157-B1: FOSSIL DEUTERATION" (2012, ApJ, 757, L9)
in The Astrophysical Journal
Parkin E
(2010)
Erratum: A 3D dynamical model of the colliding winds in binary systems
in Monthly Notices of the Royal Astronomical Society
Pineda J
(2011)
EXPANDED VERY LARGE ARRAY OBSERVATIONS OF THE BARNARD 5 STAR-FORMING CORE: EMBEDDED FILAMENTS REVEALED
in The Astrophysical Journal
Vetrov A. A.
(2008)
Fiber-optic end interferometer - a general-purpose element for constructing displacement sensors
in JOURNAL OF OPTICAL TECHNOLOGY
Bacmann A
(2010)
First detection of ND in the solar-mass protostar IRAS16293-2422
in Astronomy and Astrophysics
Caselli P
(2012)
FIRST DETECTION OF WATER VAPOR IN A PRE-STELLAR CORE
in The Astrophysical Journal
Bayet E
(2011)
First observations of CN (2-1), HCO+ (3-2) and C2H (3-2) emission lines in the Perseus cluster: constraints on heating mechanisms in the cluster gas Molecules as heating probe in Perseus
in Monthly Notices of the Royal Astronomical Society
Nazé Y
(2011)
GLOBAL X-RAY PROPERTIES OF THE O AND B STARS IN CARINA
in The Astrophysical Journal Supplement Series
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 |