CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: Dependence on redshift, halo mass, and radius

S. Roca-Fàbrega, A. Dekel, Y. Faerman, O. Gnat, C. Strawn, D. Ceverino, J. Primack, Andrea Maccio, A. A. Dutton, J. X. Prochaska, J. Stern

Research output: Contribution to journalArticle

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 by photoionization versus collisional ionization, as a function of halo mass, redshift, and distance from the galaxy halo centre. This is done utilizing two different suites of zoom-in hydro-cosmological simulations, VELA (6 haloes; z > 1) and NIHAO (18 haloes; to z = 0), which provide a broad theoretical basis because they use different codes and physical recipes for star formation and feedback. In all haloes studied in this work, we find that collisional ionization by thermal electrons dominates at high redshift, while photoionization of cool or warm gas by the metagalactic radiation takes over near z ∼ 2. In haloes of ∼1012 M and above, collisions become important again at z < 0.5, while photoionization remains significant down to z = 0 for less massive haloes. In haloes with Mv > 3 × 1011 M, at z ∼ 0 most of the photoionized OVI is in a warm, not cool, gas phase (T 3 × 105 K). We also find that collisions are dominant in the central regions of haloes, while photoionization is more significant at the outskirts, around Rv, even in massive haloes. This too may be explained by the presence of warm gas or, in lower mass haloes, by cool gas inflows.

Original languageEnglish (US)
Pages (from-to)3625-3645
Number of pages21
JournalMonthly Notices of the Royal Astronomical Society
Volume484
Issue number3
DOIs
StatePublished - Apr 11 2019

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halos
ionization
radii
gas
simulation
collision
photoionization
gases
inflow
galaxies
collisions
electron
high temperature gases
star formation
vapor phases
radiation
electrons

Keywords

  • Galaxies: evolution
  • Galaxies: formation
  • Methods: numerical

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism : Dependence on redshift, halo mass, and radius. / Roca-Fàbrega, S.; Dekel, A.; Faerman, Y.; Gnat, O.; Strawn, C.; Ceverino, D.; Primack, J.; Maccio, Andrea; Dutton, A. A.; Prochaska, J. X.; Stern, J.

In: Monthly Notices of the Royal Astronomical Society, Vol. 484, No. 3, 11.04.2019, p. 3625-3645.

Research output: Contribution to journalArticle

Roca-Fàbrega, S, Dekel, A, Faerman, Y, Gnat, O, Strawn, C, Ceverino, D, Primack, J, Maccio, A, Dutton, AA, Prochaska, JX & Stern, J 2019, 'CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: Dependence on redshift, halo mass, and radius', Monthly Notices of the Royal Astronomical Society, vol. 484, no. 3, pp. 3625-3645. https://doi.org/10.1093/mnras/stz063
Roca-Fàbrega, S. ; Dekel, A. ; Faerman, Y. ; Gnat, O. ; Strawn, C. ; Ceverino, D. ; Primack, J. ; Maccio, Andrea ; Dutton, A. A. ; Prochaska, J. X. ; Stern, J. / CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism : Dependence on redshift, halo mass, and radius. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 484, No. 3. pp. 3625-3645.
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AU - Faerman, Y.

AU - Gnat, O.

AU - Strawn, C.

AU - Ceverino, D.

AU - Primack, J.

AU - Maccio, Andrea

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