Journal article
Models of rotating coronae
- Abstract:
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Fitting equilibrium dynamical models to observational data is an essential step in understanding the structure of the gaseous hot haloes that surround our own and other galaxies. However, the two main categories of models that are used in the literature are poorly suited for this task: (i) simple barotropic models are analytic and can therefore be adjusted to match the observations, but are clearly unrealistic because the rotational velocity vϕ(R, z) does not depend on the distance z from th...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Version of record, pdf, 8.1MB)
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- Publisher copy:
- 10.1093/mnras/sty2500
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Authors
Funding
Bibliographic Details
- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 481
- Issue:
- 3
- Pages:
- 3370-3381
- Publication date:
- 2018-09-14
- Acceptance date:
- 2018-09-10
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- Source identifiers:
-
967549
Item Description
- Keywords:
- Pubs id:
-
pubs:967549
- UUID:
-
uuid:3a835a88-0a9d-46a2-bd63-d3b845a8a459
- Local pid:
- pubs:967549
- Deposit date:
- 2019-12-17
Terms of use
- Copyright holder:
- Sormani et al
- Copyright date:
- 2018
- Notes:
- © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.
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