CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass, and radius
ABSTRACT. We study the components of cool and warm/hot gas in the circumgalactic medium (CGM) of simulated galaxies and address the relative production of OVI
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
APR 2019
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2019, Volume: 484, Issue: 3, Pages: 3625-3645 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz063 |
| Online Access: | Verlag, Volltext: https://doi.org/10.1093/mnras/stz063 Verlag, Volltext: https://academic.oup.com/mnras/article/484/3/3625/5287982 
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| Author Notes: | S. Roca-Fàbrega, A. Dekel, Y. Faerman, O. Gnat, C. Strawn, D. Ceverino, J. Primack, A.V. Macciò, A.A. Dutton, J.X. Prochaska, J. Stern |
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| 245 | 1 | 0 | |a CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism |b dependence on redshift, halo mass, and radius |c S. Roca-Fàbrega, A. Dekel, Y. Faerman, O. Gnat, C. Strawn, D. Ceverino, J. Primack, A.V. Macciò, A.A. Dutton, J.X. Prochaska, J. Stern |
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