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
Caselli P
(2010)
Water vapor toward starless cores: The Herschel view
in Astronomy and Astrophysics
Caselli P
(2012)
Our astrochemical heritage
in The Astronomy and Astrophysics Review
Caswell J
(2010)
The 6-GHz methanol multibeam maser catalogue - I. Galactic Centre region, longitudes 345° to 6° Methanol maser catalogue: Galactic Centre
in Monthly Notices of the Royal Astronomical Society
Cazaux S
(2010)
Water formation on bare grains: When the chemistry on dust impacts interstellar gas
in Astronomy & Astrophysics
Cazaux S
(2011)
INTERSTELLAR ICES AS WITNESSES OF STAR FORMATION: SELECTIVE DEUTERATION OF WATER AND ORGANIC MOLECULES UNVEILED
in The Astrophysical Journal
Cazaux S
(2008)
The role of carbon grains in the deuteration of H 2
in Astronomy & Astrophysics
Ceccarelli C
(2010)
Herschel spectral surveys of star-forming regions Overview of the 555-636 GHz range
in Astronomy and Astrophysics
Chavarría L
(2010)
Water in massive star-forming regions: HIFI observations of W3 IRS5
in Astronomy and Astrophysics
Codella C
(2010)
The CHESS spectral survey of star forming regions: Peering into the protostellar shock L1157-B1 I. Shock chemical complexity
in Astronomy and Astrophysics
Codella C
(2012)
THE HERSCHEL AND IRAM CHESS SPECTRAL SURVEYS OF THE PROTOSTELLAR SHOCK L1157-B1: FOSSIL DEUTERATION
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 | 04/2011 |
End | 03/2014 |