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
Townsley L
(2011)
AN INTRODUCTION TO THE CHANDRA CARINA COMPLEX PROJECT
in The Astrophysical Journal Supplement Series
Vetrov A. A.
(2011)
Analysis and optimization of the parameters of a fiber-optic interference microphone
in JOURNAL OF OPTICAL TECHNOLOGY
Lagadec E
(2011)
A double detached shell around a post-red supergiant: IRAS 17163-3907, the Fried Egg nebula
in Astronomy & Astrophysics
Parkin E
(2011)
X-RAY EMISSION FROM THE DOUBLE-BINARY OB-STAR SYSTEM QZ CAR (HD 93206)
in The Astrophysical Journal Supplement Series
Fahed R
(2011)
Spectroscopy of the archetype colliding-wind binary WR 140 during the 2009 January periastron passage WR 140: 2009 January periastron passage
in Monthly Notices of the Royal Astronomical Society
MendigutÃa I
(2011)
Accretion rates and accretion tracers of Herbig Ae/Be stars
in Astronomy & Astrophysics
Walsh A
(2011)
The H2O Southern Galactic Plane Survey (HOPS) - I. Techniques and H2O maser data HOPS I: Techniques and H2O masers
in Monthly Notices of the Royal Astronomical Society
Oudmaijer R
(2011)
X-shooting Herbig Ae/Be stars: Accretion probed by near-infrared He I emission
in Astronomische Nachrichten
Ilee J
(2011)
Chemistry in a gravitationally unstable protoplanetary disc Chemistry in a gravitationally unstable disc
in Monthly Notices of the Royal Astronomical Society
Mottram J
(2011)
THE RMS SURVEY: THE LUMINOSITY FUNCTIONS AND TIMESCALES OF MASSIVE YOUNG STELLAR OBJECTS AND COMPACT H II REGIONS
in The Astrophysical Journal
| 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 | 03/2011 |
| End | 03/2014 |