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Dynamical models of the Milky Way

Lead Research Organisation: University of Oxford
Department Name: Oxford Physics

Abstract

Early next decade a European satellite will conduct a vast survey of our Galaxy with the goal of understanding how the Galaxy works and how it was assembled. The cuccess of this enterprise depends on our having computer models of the Galaxy that we can `survey' in the way the satellite is going to survey the Galaxy. This proposal is to use a new technology to construct such models, and use them to predict what the satellite will see.

Publications

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Hamilton C (2018) Revisiting relaxation in globular clusters in Monthly Notices of the Royal Astronomical Society

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Fulbright J (2010) THE RAVE SURVEY: RICH IN VERY METAL-POOR STARS 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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Featherstone K (2015) Greece: Greek politics stall research reforms. in Nature

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Eyre A (2009) Locating the orbits delineated by tidal streams in Monthly Notices of the Royal Astronomical Society

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

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Eyre A (2011) The mechanics of tidal streams The mechanics of tidal streams in Monthly Notices of the Royal Astronomical Society

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Das P (2016) Characterizing stellar halo populations - I. An extended distribution function for halo K giants 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 09/2009 
End 09/2012
 
Description Talks to schools 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach Local
Primary Audience Schools
Results and Impact Reported under another grant

NA
Year(s) Of Engagement Activity 2009,2010,2011,2012,2013,2014