Signatures of gas flows – II. Connecting the kinematics of the multiphase circumgalactic medium to galaxy rotation Article Swipe

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Hasti Nateghi , Glenn G. Kacprzak , Nikole M. Nielsen , Sameer Sameer , M. T. Murphy , Christopher W. Churchill , Jane C. Charlton ·

YOU? · · 2024 · Open Access · · DOI: https://doi.org/10.1093/mnras/stae2129

The multiphase circumgalactic medium (CGM) hosts critical processes that affect galaxy evolution such as accretion and outflows. We searched for evidence of these phenomena by using the EW co-rotation fraction ($f_{\rm EWcorot}$) to study the kinematic connection between the multiphase CGM and host galaxy rotation. We examined CGM absorption from Hubble Space Telescope /Cosmic Origins Spectrograph (including, but not limited to, Si ii, C ii, Si iii, C iii, and O vi) within $21\le D\le ~276$ kpc of 27 galaxies. We find the median $f_{\rm EWcorot}$ for all ions is consistent within errors and the $f_{\rm EWcorot}$ increases with increasing N$({{{\rm H} \rm{\small I}}})$. The $f_{\rm EWcorot}$ of lower ionization gas decreases with increasing $D/R_{\rm vir}$, while O vi and H i are consistent with being flat. The $f_{\rm EWcorot}$ varies minimally as a function of azimuthal angle and is similar for all ions at a fixed azimuthal angle. The larger number of O vi detections enabled us to investigate where the majority of co-rotating gas is found. Highly co-rotating O vi primarily resides along the galaxies’ major axis. Looking at the $f_{\rm EWcorot}$ as a function of ionization potential (${{\rm d}{({f_{\rm EWcorot}})}}/{{\rm d}{(\rm eV)}}$), we find a stronger co-rotation signature for lower ionization gas. There are suggestions of a connection between the CGM metallicity and major axis co-rotation where low-ionization gas with higher $f_{\rm EWcorot}$ exhibits lower metallicity and may trace large-scale filamentary inflows. Higher ionization gas with higher $f_{\rm EWcorot}$ exhibits higher metallicity and may instead trace co-planar recycled gas accretion. Our results stress the importance of comparing absorption originating from a range of ionization phases to differentiate between various gas flow scenarios.

Related Topics

Galaxy Rotation Curve

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Physics Kinematics Galaxy Astrophysics Rotation (mathematics) Galaxy rotation curve Intergalactic medium Astronomy Interstellar medium Galaxy formation and evolution Classical mechanics Geometry Redshift Mathematics

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Type: article
Language: en
Landing Page: https://doi.org/10.1093/mnras/stae2129
OA Status: gold
Cited By: 3
References: 108
Related Works: 10
OpenAlex ID: https://openalex.org/W4402543622

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DOI: https://doi.org/10.1093/mnras/stae2129

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Title: Signatures of gas flows – II. Connecting the kinematics of the multiphase circumgalactic medium to galaxy rotation

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Language: en

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Publication year: 2024

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Publication date: 2024-09-12

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Authors: Hasti Nateghi, Glenn G. Kacprzak, Nikole M. Nielsen, Sameer Sameer, M. T. Murphy, Christopher W. Churchill, Jane C. Charlton

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Landing page: https://doi.org/10.1093/mnras/stae2129

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Concepts: Physics, Kinematics, Galaxy, Astrophysics, Rotation (mathematics), Galaxy rotation curve, Intergalactic medium, Astronomy, Interstellar medium, Galaxy formation and evolution, Classical mechanics, Geometry, Redshift, Mathematics

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Cited by: 3

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