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
Meru F
(2011)
On the fragmentation criteria of self-gravitating protoplanetary discs Fragmentation criteria in discs
in Monthly Notices of the Royal Astronomical Society
Patience J
(2011)
Spatially resolved submillimeter imaging of the HR 8799 debris disk
in Astronomy & Astrophysics
Bonnell I
(2011)
The efficiency of star formation in clustered and distributed regions Clustered and distributed star formation
in Monthly Notices of the Royal Astronomical Society
Bate M
(2011)
Collapse of a molecular cloud core to stellar densities: the formation and evolution of pre-stellar discs Formation and evolution of pre-stellar discs
in Monthly Notices of the Royal Astronomical Society
Meru F
(2010)
Exploring the conditions required to form giant planets via gravitational instability in massive protoplanetary discs Giant planet formation in self-gravitating discs
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
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
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
Moeckel N
(2010)
On the evolution of a star cluster and its multiple stellar systems following gas dispersal Star cluster evolution following gas dispersal
in Monthly Notices of the Royal Astronomical Society
Rundle D
(2010)
Three-dimensional molecular line transfer: a simulated star-forming region Three-dimensional molecular line transfer
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 |