Journal article
Self-consistent modelling of the Milky Way’s nuclear stellar disc
- Abstract:
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The nuclear stellar disc (NSD) is a flattened high-density stellar structure that dominates the gravitational field of the Milky Way at Galactocentric radius $30\, {\rm pc}\lesssim R\lesssim 300\, {\rm pc}$. We construct axisymmetric self-consistent equilibrium dynamical models of the NSD in which the distribution function is an analytic function of the action variables. We fit the models to the normalized kinematic distributions (line-of-sight velocities + VIRAC2 proper motions) of...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Accepted manuscript, 4.0MB)
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- Publisher copy:
- 10.1093/mnras/stac639
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Authors
Bibliographic Details
- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 512
- Issue:
- 2
- Pages:
- 1857-1884
- Publication date:
- 2022-03-22
- Acceptance date:
- 2022-03-04
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
Item Description
- Language:
- English
- Keywords:
- Pubs id:
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1248861
- Local pid:
- pubs:1248861
- Deposit date:
- 2022-03-30
Terms of use
- Copyright holder:
- Sormani et al.
- Copyright date:
- 2022
- Rights statement:
- © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
- Notes:
-
This is the accepted manuscript version of the article. The final version is available from Oxford University Press at https://doi.org/10.1093/mnras/stac639
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