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.

Publications

10 25 50

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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,

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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,

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Williams M (2011) THE DAWNING OF THE STREAM OF AQUARIUS IN RAVE in The Astrophysical Journal

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Sharma S (2011) GALAXIA: A CODE TO GENERATE A SYNTHETIC SURVEY OF THE MILKY WAY in The Astrophysical Journal

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Fouvry J (2015) SELF-GRAVITY, RESONANCES AND ORBITAL DIFFUSION IN STELLAR DISKS in The Astrophysical Journal

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Fulbright J (2010) THE RAVE SURVEY: RICH IN VERY METAL-POOR STARS in The Astrophysical Journal

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Siebert A (2011) THE RADIAL VELOCITY EXPERIMENT (RAVE): THIRD DATA RELEASE in The Astronomical Journal

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Kordopatis G (2013) THE RADIAL VELOCITY EXPERIMENT (RAVE): FOURTH DATA RELEASE in The Astronomical Journal

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Matijevic G (2010) DOUBLE-LINED SPECTROSCOPIC BINARY STARS IN THE RAVE SURVEY in The Astronomical Journal

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Monari G (2018) Distribution functions for resonantly trapped orbits in our Galaxy in Proceedings of the International Astronomical Union

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Cole D (2018) Self-consistent Modelling of the Milky Way using Gaia data in Proceedings of the International Astronomical Union

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Binney J (2020) Modelling our galaxy in Proceedings of the International Astronomical Union

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Sanders J (2014) Stream-orbit misalignment & a new algorithm for constraining the Galactic potential with streams in Proceedings of the International Astronomical Union

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Binney J (2014) Dynamical models and Galaxy surveys in Proceedings of the International Astronomical Union

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Binney J (2013) Dynamics for galactic archaeology in New Astronomy Reviews

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Featherstone K (2015) Greece: Greek politics stall research reforms. in Nature

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Eyre A (2009) Fitting orbits to tidal streams with proper motions in Monthly Notices of the Royal Astronomical Society: Letters

 
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