Journal article

Self-consistent modelling of our Galaxy with Gaia data

Abstract:: Galaxy models are fundamental to exploiting surveys of our Galaxy. There is now a significant body of work on axisymmetric models. A model can be defined by giving the DF of each major class of stars and of dark matter. Then the self-consistent gravitational potential is determined. Other modelling techniques are briefly considered before an overview of some early work on non-axisymmetric models.

Publication status:: Published

Peer review status:: Peer reviewed

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APA Style

Binney, J. (2018). Self-consistent modelling of our Galaxy with Gaia data. Proceedings of the International Astronomical Union, 12, 111–118.

MLA Style

Binney, J. “Self-Consistent Modelling of Our Galaxy with Gaia Data.” Proceedings of the International Astronomical Union, vol. 12, Cambridge University Press, 2018, pp. 111–18.

Chicago Style

Binney, J. 2018. “Self-Consistent Modelling of Our Galaxy with Gaia Data.” Proceedings of the International Astronomical Union 12: 111–18.
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Files:: 1706.01374v1.pdf

(Preview, Accepted manuscript, pdf, 150.1KB, Terms of use)

Publisher copy:: 10.1017/S1743921317007049

Authors

+ Binney, J More by this author

Institution:: University of Oxford
Division:: MPLS
Department:: Physics
Sub department:: Theoretical Physics
Oxford college:: Merton College
Role:: Author

+ Science and Technology Facilities Council More from this funder

Grant:: ST/G002509/1

Publisher:: Cambridge University Press
Journal:: Proceedings of the International Astronomical Union More from this journal
Volume:: 12
Pages:: 111-118
Publication date:: 2018-03-07
Acceptance date:: 2016-12-23
DOI:: 10.1017/S1743921317007049
EISSN:: 1743-9221
ISSN:: 1743-9213

Keywords:: Galaxy: kinematics and dynamics

stellar dynamics

(cosmology:) dark matter
Pubs id:: pubs:797940
UUID:: uuid:518ceb8c-058e-42df-aa57-35d45d0e123f
Local pid:: pubs:797940
Source identifiers:: 797940
Deposit date:: 2018-01-23

Terms of use

Copyright holder:: International Astronomical Union
Copyright date:: 2018
Notes:: Copyright © 2018 International Astronomical Union. This paper was presented at the IAUS 330: Astrometry and Astrophysics in the Gaia Sky, 24-28 April 2017, Nice,
France. This is the accepted manuscript version of the paper. The final version is available online from Cambridge University Press at: https://doi.org/10.1017/S1743921317007049

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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