The formation of stars and planets: Radiation hydrodynamical and magnetohydrodynamical simulations
Lead Research Organisation:
UNIVERSITY OF EXETER
Department Name: Physics
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
Organisations
Publications

Dobbs C
(2008)
Simulations of spiral galaxies with an active potential: molecular cloud formation and gas dynamics
in Monthly Notices of the Royal Astronomical Society

Bate M
(2009)
Stellar, brown dwarf and multiple star properties from hydrodynamical simulations of star cluster formation
in Monthly Notices of the Royal Astronomical Society

Ayliffe B
(2009)
Circumplanetary disc properties obtained from radiation hydrodynamical simulations of gas accretion by protoplanets
in Monthly Notices of the Royal Astronomical Society

Price D
(2009)
Inefficient star formation: the combined effects of magnetic fields and radiative feedback
in Monthly Notices of the Royal Astronomical Society

Bate M
(2009)
The dependence of star formation on initial conditions and molecular cloud structure
in Monthly Notices of the Royal Astronomical Society

Ayliffe B
(2009)
Gas accretion on to planetary cores: three-dimensional self-gravitating radiation hydrodynamical calculations
in Monthly Notices of the Royal Astronomical Society

Bate M
(2009)
The importance of radiative feedback for the stellar initial mass function
in Monthly Notices of the Royal Astronomical Society

Ayliffe B
(2010)
Planet migration: self-gravitating radiation hydrodynamical models of protoplanets with surfaces Planetary migration and growth
in Monthly Notices of the Royal Astronomical Society

Bate M
(2010)
Collapse of a molecular cloud core to stellar densities: the radiative impact of stellar core formation on the circumstellar disc
in Monthly Notices of the Royal Astronomical Society: Letters

Dobbs C
(2010)
Simulations of the grand design galaxy M51: a case study for analysing tidally induced spiral structure Simulations of tidally induced structure in M51
in Monthly Notices of the Royal Astronomical Society
Description | This grant provided funding for research into star and planet formation. |
Exploitation Route | Via refereed journal articles. |
Sectors | Digital/Communication/Information Technologies (including Software) Education |
URL | http://www.astro.ex.ac.uk/people/mbate/ |
Description | Findings were published in refereed journal papers. Animations and images provided at http://www.astro.ex.ac.uk/people/mbate |
First Year Of Impact | 2006 |
Sector | Creative Economy,Education,Culture, Heritage, Museums and Collections |
Impact Types | Cultural |
Description | ERC Advanced Grant |
Amount | € 1,706,418 (EUR) |
Funding ID | No. 339248 |
Organisation | European Research Council (ERC) |
Sector | Public |
Country | Belgium |
Start | 03/2014 |
End | 02/2019 |
Description | STFC Consolidated Grant |
Amount | £1,734,000 (GBP) |
Funding ID | ST/J001627/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2012 |
End | 09/2015 |