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Theoretical physicists working at a blackboard collaboration pod in the Beecroft building.
Credit: Jack Hobhouse

Professor James Binney FRS

Emeritus Professor

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Theoretical astrophysics and plasma physics at RPC
James.Binney@physics.ox.ac.uk
Telephone: 01865 (2)73979
Rudolf Peierls Centre for Theoretical Physics, room 50.3
  • About
  • Publications

New distances to RAVE stars

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 437:1 (2014) 351-370

Authors:

J Binney, B Burnett, G Kordopatis, PJ McMillan, S Sharma, T Zwitter, O Bienaymé, J Bland-Hawthorn, M Steinmetz, G Gilmore, MEK Williams, J Navarro, EK Grebel, A Helmi, Q Parker, WA Reid, G Seabroke, F Watson, RFG Wyse
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A NEW STELLAR CHEMO-KINEMATIC RELATION REVEALS THE MERGER HISTORY OF THE MILKY WAY DISK

ASTROPHYSICAL JOURNAL LETTERS 781:1 (2014) ARTN L20

Authors:

I Minchev, C Chiappini, M Martig, M Steinmetz, RS de Jong, C Boeche, C Scannapieco, T Zwitter, RFG Wyse, JJ Binney, J Bland-Hawthorn, O Bienayme, B Famaey, KC Freeman, BK Gibson, EK Grebel, G Gilmore, A Helmi, G Kordopatis, YS Lee, U Munari, JF Navarro, QA Parker, AC Quillen, WA Reid, A Siebert, A Siviero, G Seabroke, F Watson, M Williams
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The radial velocity experiment (RAVE): Fourth data release

Astronomical Journal 146:5 (2013)

Authors:

G Kordopatis, G Gilmore, M Steinmetz, C Boeche, GM Seabroke, A Siebert, T Zwitter, J Binney, P De Laverny, A Recio-Blanco, MEK Williams, T Piffl, H Enke, S Roeser, A Bijaoui, RFG Wyse, K Freeman, U Munari, I Carrillo, B Anguiano, D Burton, R Campbell, CJP Cass, K Fiegert, M Hartley, QA Parker, W Reid, A Ritter, KS Russell, M Stupar, FG Watson, O Bienaymé, J Bland-Hawthorn, O Gerhard, BK Gibson, EK Grebel, A Helmi, JF Navarro, C Conrad, B Famaey, C Faure, A Just, J Kos, G Matijevič, PJ McMillan, I Minchev, R Scholz, S Sharma, A Siviero, E Wylie De Boer, M Žerjal

Abstract:

We present the stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, individual abundances, and distances determined for 425,561 stars, which constitute the fourth public data release of the RAdial Velocity Experiment (RAVE). The stellar atmospheric parameters are computed using a new pipeline, based on the algorithms of MATISSE and DEGAS. The spectral degeneracies and the Two Micron All Sky Survey photometric information are now better taken into consideration, improving the parameter determination compared to the previous RAVE data releases. The individual abundances for six elements (magnesium, aluminum, silicon, titanium, iron, and nickel) are also given, based on a special-purpose pipeline that is also improved compared to that available for the RAVE DR3 and Chemical DR1 data releases. Together with photometric information and proper motions, these data can be retrieved from the RAVE collaboration Web site and the Vizier database. © 2013. The American Astronomical Society. All rights reserved.
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Stream–orbit misalignment – I. The dangers of orbit-fitting

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 433:3 (2013) 1813-1825

Authors:

Jason L Sanders, James Binney
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Stream–orbit misalignment – II. A new algorithm to constrain the Galactic potential

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 433:3 (2013) 1826-1836

Authors:

Jason L Sanders, James Binney
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