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1
Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab2933
Abstract: We present the first characterization of the circumgalactic medium of Lyα emitters (LAEs), using a sample of 96 z ≈ 3.3 LAEs detected with the VLT/MUSE in fields centered on 8 bright background quasars. The…
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Keywords:
absorption;
medium;
circumgalactic medium;
musequbes characterizing ... See more keywords
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1
Published in 2022 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stac2390
Abstract: Motivated by integral field units (IFUs) on large ground telescopes and proposals for ultraviolet-sensitive space telescopes to probe circumgalactic medium (CGM) emission, we survey the most promising emission lines and how such observations can inform…
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Keywords:
circumgalactic medium;
gas;
emission estimates;
emission ... See more keywords
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3
Published in 2023 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad1195
Abstract: We study the impact of resonantly scattered X-ray line emission on the observability of the hot circumgalactic medium (CGM) of galaxies. We apply a Monte Carlo radiative transfer post-processing analysis to the high-resolution TNG50 cosmological…
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Keywords:
cgm;
circumgalactic medium;
resonant scattering;
ray emission ... See more keywords
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0
Published in 2025 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staf1372
Abstract: Galaxy evolution is shaped by star formation and stellar feedback at scales unresolved by current high-resolution cosmological simulations. Precise subgrid models are thus necessary, and different approaches have been developed. However, they are degenerate and…
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Keywords:
mechanical feedback;
circumgalactic medium;
feedback;
model ... See more keywords
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Published in 2024 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staf786
Abstract: The circumgalactic medium (CGM) in ≳ 1012 M⊙ halos is dominated by a hot phase (T ≳ 106 K). While many models exist for the hot gas structure, there is as yet no consensus. We compare…
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Keywords:
circumgalactic medium;
cooling flows;
cgm;
halos ... See more keywords
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1
Published in 2017 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stx2968
Abstract: Annihilating dark matter (DM) models offer promising avenues for future DM detection, in particular via modification of astrophysical signals. However when modelling such potential signals at high redshift the emergence of both dark matter and…
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Keywords:
annihilation;
energy;
matter;
dark matter ... See more keywords
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1
Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty1283
Abstract: We characterize the properties of the intergalactic medium (IGM) around a sample of galaxies extracted from state-of-the-art hydrodynamical simulations of structure formation in a cosmological volume of 25 Mpc comoving at $z\sim 2$. The simulations…
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Keywords:
absorption systems;
medium;
circumgalactic medium;
probe circumgalactic ... See more keywords
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1
Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz1773
Abstract: We use a particle tracking analysis to study the origins of the circumgalactic medium (CGM), separating it into (1) accretion from the intergalactic medium (IGM), (2) wind from the central galaxy, and (3) gas ejected…
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Keywords:
medium;
circumgalactic medium;
origins circumgalactic;
gas ... See more keywords
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0
Published in 2018 at "Monthly Notices of the Royal Astronomical Society: Letters"
DOI: 10.1093/mnrasl/sly190
Abstract: The circumgalactic medium (CGM), i.e. the gaseous haloes around galaxies, is both the reservoir of gas that fuels galaxy growth and the repository of gas expelled by galactic winds. Most cosmological, hydrodynamical simulations focus their…
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Keywords:
resolution;
column;
circumgalactic medium;
cosmological simulations ... See more keywords
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0
Published in 2025 at "Journal of Astronomical Telescopes, Instruments, and Systems"
DOI: 10.1117/1.jatis.11.4.042213
Abstract: Abstract. We present a science case for the Habitable Worlds Observatory (HWO) to map the circumgalactic medium (CGM) in emission by targeting ultraviolet emission lines, which trace the 104 to 106 K gas engaged in the…
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Keywords:
spectroscopy;
worlds observatory;
habitable worlds;
circumgalactic medium ... See more keywords
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0
Published in 2024 at "Science Advances"
DOI: 10.1126/sciadv.adp8629
Abstract: The recent detection of optical emission lines from the circumgalactic medium (CGM) in combined, large samples of low-redshift, normal galaxy spectra hints at the potential to map the cool (∼104 kelvin) CGM in individual, representative…
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Keywords:
circumgalactic medium;
source blind;
galaxy;
emission ... See more keywords