Models of rotating coronae
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 ba...
| Main Authors: | , , , , |
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| Format: | Journal article |
| Published: |
Oxford University Press
2018
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