Dynamical models of the milky way
Lead Research Organisation:
University of Oxford
Department Name: Oxford Physics
Abstract
A huge investment is currently being made in surveys of stars in our Galaxy. From the motions of these stars we can in principle determine the distribution in the Galaxy of the mysterious dark matter that comprises more than 80% of the matter in the Universe. From the motions of stars we also expect to be able to reconstruct the way the Galaxy was assembled from smaller units that merged together. To achieve these goals we need sophistcated dynamical models and software that enables us to assess how likely a model is given the measured data. This grant funds the construction of such models and software, and early applications to data from ground-based observatories. Eventually the models will be used to extract the science goals of the European Space Agency's 'Cornerstone Mission' Gaia, which will measure the positions and velocities of a billion stars.
People |
ORCID iD |
| James Binney (Principal Investigator) |
Publications
Binney J
(2014)
Dynamical models and Galaxy surveys
in Proceedings of the International Astronomical Union
Matijevic G
(2010)
DOUBLE-LINED SPECTROSCOPIC BINARY STARS IN THE RAVE SURVEY
in The Astronomical Journal
Binney J
(2010)
Distribution functions for the Milky Way
in Monthly Notices of the Royal Astronomical Society
Monari G
(2017)
Distribution functions for resonantly trapped orbits in the Galactic disc
in Monthly Notices of the Royal Astronomical Society
Monari G
(2018)
Distribution functions for resonantly trapped orbits in our Galaxy
in Proceedings of the International Astronomical Union
Famaey B
(2018)
Distribution functions for Galactic disc stellar populations in the presence of non-axisymmetric perturbations
in Proceedings of the International Astronomical Union
Burnett B
(2011)
Distance determination for RAVE stars using stellar models III. The nature of the RAVE survey and Milky Way chemistry
in Astronomy & Astrophysics
Zwitter T
(2010)
Distance determination for RAVE stars using stellar models II. Most likely values assuming a standard stellar evolution scenario*
in Astronomy & Astrophysics
Breddels M
(2010)
Distance determination for RAVE stars using stellar models
in Astronomy and Astrophysics
Kos J
(2013)
DIFFUSE INTERSTELLAR BAND AT 8620 Å IN RAVE: A NEW METHOD FOR DETECTING THE DIFFUSE INTERSTELLAR BAND IN SPECTRA OF COOL STARS
in The Astrophysical Journal
| Description | STFC studentships |
| Amount | £35,000 (GBP) |
| Organisation | Science and Technologies Facilities Council (STFC) |
| Sector | Public |
| Country | United Kingdom |
| Start | 09/2009 |
| End | 09/2012 |
| Description | A new generation of Galaxy models |
| Organisation | Max Planck Society |
| Department | Max Planck Institute For Extraterrestrial Physics (MPE) |
| Country | Germany |
| Sector | Academic/University |
| PI Contribution | Expertise in dynamical modelling |
| Collaborator Contribution | Participation in several worthwhile papers |
| Impact | The paper Sharma et al in the publications list. Also a contribution to a paper Burnett et al that has been submitted & is under review |
| Start Year | 2010 |
| Description | A new generation of Galaxy models |
| Organisation | University of Sydney |
| Department | School of Physics |
| Country | Australia |
| Sector | Academic/University |
| PI Contribution | Expertise in dynamical modelling |
| Collaborator Contribution | Participation in several worthwhile papers |
| Impact | The paper Sharma et al in the publications list. Also a contribution to a paper Burnett et al that has been submitted & is under review |
| Start Year | 2010 |
| Description | Galactic fountains and gas accretion |
| Organisation | University of Bologna |
| Department | Department of Physics and Astronomy |
| Country | Italy |
| Sector | Academic/University |
| PI Contribution | Expertise in dynamical modelling and in the theory of the intergalactic medium |
| Collaborator Contribution | Fellowships to suport work in Oxford by colleagues from Bologna and through this participation in several publications (only 1 of these appeared after the grant start date and a further one has been submitted & is under review) |
| Impact | Several well-cited papers |
| Description | Modelling the chemodynamical evolution of the Milky Way |
| Organisation | Max Planck Society |
| Department | Max Planck Institute For Extraterrestrial Physics (MPE) |
| Country | Germany |
| Sector | Academic/University |
| PI Contribution | Expertise in dynamical modelling |
| Collaborator Contribution | Participation in significant papers |
| Impact | We have published three joint papers so far (two in the publication list, one appeared before the grant start date) and several in preparation. These are already widely cited papers |
| Start Year | 2007 |
| Description | School visit |
| Form Of Engagement Activity | Participation in an open day or visit at my research institution |
| Part Of Official Scheme? | No |
| Geographic Reach | Regional |
| Primary Audience | Schools |
| Results and Impact | I regularly give talks at schools. Sometimes it is to the Physics Society, sometimes it is a talk to 6th formers (although younger pupils often attend too). There are always lots of good questions. Nothing to report |
| Year(s) Of Engagement Activity | 2009,2010,2011,2012,2013,2014 |
| Description | Talks to local astronomy clubs |
| Form Of Engagement Activity | A talk or presentation |
| Part Of Official Scheme? | No |
| Geographic Reach | Regional |
| Primary Audience | Public/other audiences |
| Results and Impact | These events usually attract ~30 people with a wide range of educational backgrounds. There are always plenty of questions, some quite shrewd. Nothing to report |
| Year(s) Of Engagement Activity | 2006,2007,2008,2009,2011 |