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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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

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McMillan P (2013) Analysing surveys of our Galaxy - II. Determining the potential in Monthly Notices of the Royal Astronomical Society

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Binney J (2020) Angle-action variables for orbits trapped at a Lindblad resonance in Monthly Notices of the Royal Astronomical Society

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Piffl T (2015) Bringing the Galaxy's dark halo to life 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

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Das P (2016) Characterizing stellar halo populations II: the age gradient in blue horizontal-branch stars in Monthly Notices of the Royal Astronomical Society

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Binney James (2015) Chemodynamical modelling of the Milky Way in ArXiv e-prints

 
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 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