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
Coppin K
(2012)
Herschel -PACS observations of [O i ]63 µm towards submillimetre galaxies at z ~ 1 Herschel observations of [O i ]63 µ m in z ~ 1 SMGs
in Monthly Notices of the Royal Astronomical Society
Codella C
(2012)
THE HERSCHEL AND IRAM CHESS SPECTRAL SURVEYS OF THE PROTOSTELLAR SHOCK L1157-B1: FOSSIL DEUTERATION
in The Astrophysical Journal
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
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
Chavarría L
(2010)
Water in massive star-forming regions: HIFI observations of W3 IRS5
in Astronomy and Astrophysics
Ceccarelli C
(2010)
Herschel spectral surveys of star-forming regions Overview of the 555-636 GHz range
in Astronomy and Astrophysics
Cazaux S
(2008)
The role of carbon grains in the deuteration of H 2
in Astronomy & Astrophysics
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
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
Caselli P
(2012)
Our astrochemical heritage
in The Astronomy and Astrophysics Review
Caselli P
(2010)
Water vapor toward starless cores: The Herschel view
in Astronomy and Astrophysics
Caselli P
(2008)
Survey of ortho-H$\mathsf{_{2}}$D$\mathsf{^{+}}$ (1$\mathsf{_{1,0}}$-1$\mathsf{_{1,1}}$) in dense cloud cores
in Astronomy & Astrophysics
Caselli P
(2012)
FIRST DETECTION OF WATER VAPOR IN A PRE-STELLAR CORE
in The Astrophysical Journal
Camus N
(2009)
Observations of â??wispsâ?? in magnetohydrodynamic simulations of the Crab Nebula
in Monthly Notices of the Royal Astronomical Society
Bruderer S
(2010)
Herschel /HIFI detections of hydrides towards AFGL 2591 Envelope emission versus tenuous cloud absorption
in Astronomy and Astrophysics
Bourke T
(2012)
INITIAL CONDITIONS FOR STAR FORMATION IN CLUSTERS: PHYSICAL AND KINEMATICAL STRUCTURE OF THE STARLESS CORE Oph A-N6
in The Astrophysical Journal
Bizzocchi L
(2010)
Detection of N$^\mathsf{ {15}}$NH + in L1544
in Astronomy and Astrophysics
Bergin E
(2010)
Sensitive limits on the abundance of cold water vapor in the DM Tauri protoplanetary disk
in Astronomy and Astrophysics
Benz A
(2010)
Hydrides in young stellar objects: Radiation tracers in a protostar-disk-outflow system
in Astronomy and Astrophysics
Benedettini M
(2012)
Multiline spectral imaging of dense cores in the Lupus molecular cloud Multiline spectral imaging of dense cores in Lupus
in Monthly Notices of the Royal Astronomical Society
Bayet E
(2010)
Molecular tracers of filamentary CO emission regions surrounding the central galaxies of clusters
in Astronomy and Astrophysics
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
Bayet E
(2011)
Chemistry in cosmic ray dominated regions Chemistry at high CR
in Monthly Notices of the Royal Astronomical Society
Barkov M. V.
(2008)
MAGNETIC ACCELERATION OF ULTRARELATIVISTIC GRB AND AGN JETS
in INTERNATIONAL JOURNAL OF MODERN PHYSICS D
Barkov M
(2008)
Stellar explosions powered by the Blandford-Znajek mechanism
in Monthly Notices of the Royal Astronomical Society: Letters
Barkov M
(2011)
Recycling of neutron stars in common envelopes and hypernova explosions Recycling of neutron stars and hypernovae
in Monthly Notices of the Royal Astronomical Society
Barkov M
(2010)
Close binary progenitors of gamma-ray bursts
in Monthly Notices of the Royal Astronomical Society
Bacmann A
(2010)
First detection of ND in the solar-mass protostar IRAS16293-2422
in Astronomy and Astrophysics
Ashmore I
(2010)
Transient evolution of C-type shocks in dusty regions of varying density
in Astronomy and Astrophysics
Aluzas R
(2012)
Numerical simulations of shocks encountering clumpy regions Simulations of shocks encountering clumpy regions
in Monthly Notices of the Royal Astronomical Society
Alonso-Albi T
(2010)
Chemical study of intermediate-mass (IM) Class 0 protostars CO depletion and N 2 H + deuteration
in Astronomy and Astrophysics
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 |