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 surroun
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| Main Authors: | , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
2018 September 14
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 481, Issue: 3, Pages: 3370-3381 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2500 |
| Online Access: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2500 Verlag, Volltext: https://academic.oup.com/mnras/article/481/3/3370/5097896 
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| Author Notes: | Mattia C. Sormani, Emanuele Sobacchi, Gabriele Pezzulli, James Binney and Ralf S. Klessen |
| Summary: | Fitting equilibrium dynamical models to observational data is an essential step in understanding the structure of the gaseous hot haloes that surroun |
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| Item Description: | Gesehen am 06.08.2020 |
| Physical Description: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2500 |