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
Jackson R. J.
(2015)
VizieR Online Data Catalog: Velocity precision in the Gaia-ESO Survey (Jackson+, 2015)
in VizieR Online Data Catalog
Pezzulli G.
(2016)
The angular momentum of hot coronae around spiral galaxies and its impact on the evolution of star forming discs
in The Interplay between Local and Global Processes in Galaxies,
Posti L.
(2016)
Self-consistent dynamical models for early-type galaxies in the CALIFA Survey
in The Interplay between Local and Global Processes in Galaxies,
Minchev I
(2014)
A NEW STELLAR CHEMO-KINEMATIC RELATION REVEALS THE MERGER HISTORY OF THE MILKY WAY DISK
in The Astrophysical Journal
Fouvry J
(2015)
SELF-GRAVITY, RESONANCES AND ORBITAL DIFFUSION IN STELLAR DISKS
in The Astrophysical Journal
Fulbright J
(2010)
THE RAVE SURVEY: RICH IN VERY METAL-POOR STARS
in The Astrophysical Journal
Sharma S
(2014)
KINEMATIC MODELING OF THE MILKY WAY USING THE RAVE AND GCS STELLAR SURVEYS
in The Astrophysical Journal
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
Sharma S
(2011)
GALAXIA: A CODE TO GENERATE A SYNTHETIC SURVEY OF THE MILKY WAY
in The Astrophysical Journal
Fraternali F
(2013)
IONIZED ABSORBERS AS EVIDENCE FOR SUPERNOVA-DRIVEN COOLING OF THE LOWER GALACTIC CORONA
in The Astrophysical Journal
Williams M
(2011)
THE DAWNING OF THE STREAM OF AQUARIUS IN RAVE
in The Astrophysical Journal
Ruchti G
(2010)
ORIGINS OF THE THICK DISK AS TRACED BY THE ALPHA ELEMENTS OF METAL-POOR GIANT STARS SELECTED FROM RAVE
in The Astrophysical Journal
Siebert A
(2011)
THE RADIAL VELOCITY EXPERIMENT (RAVE): THIRD DATA RELEASE
in The Astronomical Journal
Matijevic G
(2010)
DOUBLE-LINED SPECTROSCOPIC BINARY STARS IN THE RAVE SURVEY
in The Astronomical Journal
Kordopatis G
(2013)
THE RADIAL VELOCITY EXPERIMENT (RAVE): FOURTH DATA RELEASE
in The Astronomical Journal
Kos J
(2014)
Interstellar medium. Pseudo-three-dimensional maps of the diffuse interstellar band at 862 nm.
in Science (New York, N.Y.)
Famaey B
(2018)
Distribution functions for Galactic disc stellar populations in the presence of non-axisymmetric perturbations
in Proceedings of the International Astronomical Union
Sanders J
(2014)
Stream-orbit misalignment & a new algorithm for constraining the Galactic potential with streams
in Proceedings of the International Astronomical Union
Binney J
(2014)
Dynamical models and Galaxy surveys
in Proceedings of the International Astronomical Union
Binney J
(2020)
Modelling our galaxy
in Proceedings of the International Astronomical Union
Monari G
(2018)
Distribution functions for resonantly trapped orbits in our Galaxy
in Proceedings of the International Astronomical Union
Cole D
(2018)
Self-consistent Modelling of the Milky Way using Gaia data
in Proceedings of the International Astronomical Union
Binney J
(2013)
Dynamics for galactic archaeology
in New Astronomy Reviews
Featherstone K
(2015)
Greece: Greek politics stall research reforms.
in Nature
Eyre A
(2009)
Fitting orbits to tidal streams with proper motions
in Monthly Notices of the Royal Astronomical Society: Letters
McMillan P
(2009)
The dangers of deprojection of proper motions
in Monthly Notices of the Royal Astronomical Society: Letters
Binney J
(2014)
New distances to RAVE stars
in Monthly Notices of the Royal Astronomical Society
Schönrich R
(2012)
A new formula for disc kinematics A new formula for disc kinematics
in Monthly Notices of the Royal Astronomical Society
Posti L
(2015)
Action-based distribution functions for spheroidal galaxy components
in Monthly Notices of the Royal Astronomical Society
Pezzulli Gabriele
(2017)
The angular momentum of cosmological coronae and the inside-out growth of spiral galaxies
in Monthly Notices of the Royal Astronomical Society
Aumer M
(2017)
The structural evolution of galaxies with both thin and thick discs
in Monthly Notices of the Royal Astronomical Society
Eyre A
(2011)
The mechanics of tidal streams The mechanics of tidal streams
in Monthly Notices of the Royal Astronomical Society
Sanders J
(2014)
Actions, angles and frequencies for numerically integrated orbits
in Monthly Notices of the Royal Astronomical Society
Wojno J
(2017)
The selection function of the RAVE survey
in Monthly Notices of the Royal Astronomical Society
Eyre A
(2009)
Locating the orbits delineated by tidal streams
in Monthly Notices of the Royal Astronomical Society
Sanders J
(2015)
A fast algorithm for estimating actions in triaxial potentials
in Monthly Notices of the Royal Astronomical Society
Schönrich R
(2010)
Local kinematics and the local standard of rest
in Monthly Notices of the Royal Astronomical Society
Sormani M
(2015)
Gas flow in barred potentials - III. Effects of varying the quadrupole
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
Cole D
(2017)
A centrally heated dark halo for our Galaxy
in Monthly Notices of the Royal Astronomical Society
McMillan P
(2012)
Analysing surveys of our Galaxy - I. Basic astrometric data Analysing surveys of our Galaxy
in Monthly Notices of the Royal Astronomical Society
McMillan P
(2018)
Improved distances and ages for stars common to TGAS and RAVE
in Monthly Notices of the Royal Astronomical Society
Das P
(2016)
Characterizing stellar halo populations - I. An extended distribution function for halo K giants
in Monthly Notices of the Royal Astronomical Society
Binney J
(2017)
Modelling the Milky Way's globular cluster system
in Monthly Notices of the Royal Astronomical Society
Carrillo I
(2018)
Is the Milky Way still breathing? RAVE-Gaia streaming motions
in Monthly Notices of the Royal Astronomical Society
Pascale R
(2018)
Action-based dynamical models of dwarf spheroidal galaxies: application to Fornax
in Monthly Notices of the Royal Astronomical Society
Binney J
(2014)
Galactic kinematics and dynamics from Radial Velocity Experiment stars
in Monthly Notices of the Royal Astronomical Society
Lau J
(2019)
Relaxation of spherical stellar systems
in Monthly Notices of the Royal Astronomical Society
Binney J
(2011)
Models of our Galaxy - II Models of our Galaxy - II
in Monthly Notices of the Royal Astronomical Society
Wojno J
(2018)
Correlations between age, kinematics, and chemistry as seen by the RAVE survey
in Monthly Notices of the Royal Astronomical Society
| Description | STFC studentships |
| Amount | £35,000 (GBP) |
| Organisation | Science and Technologies Facilities Council (STFC) |
| Sector | Public |
| Country | United Kingdom |
| Start | 10/2009 |
| 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 |