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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

10 25 50

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Binney J (2015) The distribution function of the Galaxy's dark halo in Monthly Notices of the Royal Astronomical Society

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Sanders J (2015) Extended distribution functions for our Galaxy in Monthly Notices of the Royal Astronomical Society

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Binney James (2015) TM: Torus Mapper in Astrophysics Source Code Library

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Kordopatis G (2015) The rich are different: evidence from the RAVE survey for stellar radial migration in Monthly Notices of the Royal Astronomical Society

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Sormani M (2015) Gas flow in barred potentials - III. Effects of varying the quadrupole in Monthly Notices of the Royal Astronomical Society

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Nipoti C (2015) Early flattening of dark matter cusps in dwarf spheroidal galaxies in Monthly Notices of the Royal Astronomical Society

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Sormani M (2015) Gas flow in barred potentials - II. Bar-driven spiral arms 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