Search Results - "Peroux, Céline"
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Observed cosmic evolution of galaxy dust properties with metallicity and tensions with models
Published in Monthly notices of the Royal Astronomical Society (01-06-2022)“…ABSTRACT The dust abundance of the interstellar medium plays an important role in galaxy physics, the chemical evolution of matter, and the absorption and…”
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The Cosmic Baryon and Metal Cycles
Published in Annual review of astronomy and astrophysics (01-01-2020)“…Characterizing the relationship between stars, gas, and metals in galaxies is a critical component of understanding the cosmic baryon cycle. We compile…”
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Closing gaps to our origins
Published in Experimental astronomy (01-12-2022)“…This article reproduces the contents of the White Paper entitled by the same name submitted to the call issued by the European Space Agency soliciting ideas…”
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Closing gaps to our origins: EUVO: the ultraviolet-visible window into the Universe
Published in Experimental astronomy (01-12-2022)“…This article reproduces the contents of the White Paper entitled by the same name submitted to the call issued by the European Space Agency soliciting ideas…”
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Predictions for the angular dependence of gas mass flow rate and metallicity in the circumgalactic medium
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT We use cosmological hydrodynamical simulations to examine the physical properties of the gas in the circumgalactic media (CGM) of star-forming…”
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Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
Published in Monthly notices of the Royal Astronomical Society (01-12-2021)“…ABSTRACT We contrast the latest observations of the cosmic metal density in neutral gas ($\rho _{ {met,neu}}$) with three cosmological galaxy evolution…”
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Late-time cosmic evolution of dust: solving the puzzle
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT Dust is an essential ingredient of galaxies, determining the physical and chemical conditions in the interstellar medium. Several complementary…”
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Observed dust surface density across cosmic times
Published in Monthly notices of the Royal Astronomical Society (11-05-2023)“…ABSTRACT Our ability to interpret observations of galaxies and trace their stellar, gas, and dust content over cosmic time critically relies on our…”
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Nature of the absorbing gas associated with a galaxy group at z∼0.4
Published in Monthly notices of the Royal Astronomical Society (11-01-2017)“…We present new Multi Unit Spectroscopic Explorer observations of quasar field Q2131-1207 with a log N(HI)N(HI) = 19.50 ± 0.15 sub-damped Lyman a at zabs =…”
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A SINFONI integral field spectroscopy survey for galaxy counterparts to damped Lyman α systems - III. Three additional detections
Published in Monthly notices of the Royal Astronomical Society (01-02-2012)“…We report three additional Spectrograph for Integral Field Observations in the Near Infrared (SINFONI) detections of Hα emission line from quasar absorbers,…”
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Clumpiness of observed and simulated cold circumgalactic gas
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT Determining the clumpiness of matter around galaxies is pivotal to a full understanding of the spatially inhomogeneous, multiphase gas in the…”
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A SINFONI integral field spectroscopy survey for galaxy counterparts to damped Lyman α systems - I. New detections and limits for intervening and associated absorbers
Published in Monthly notices of the Royal Astronomical Society (01-02-2011)“…Detailed studies of damped and sub-damped Lyman α systems (DLAs), the galaxies probed by the absorption they produce in the spectra of background quasars, rely…”
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A SINFONI integral field spectroscopy Survey for galaxy counterparts to Damped Lyman α Systems - V. Neutral and ionized-phase metallicities
Published in Monthly notices of the Royal Astronomical Society (01-02-2014)“…The gas-phase and stellar metallicities have proven to be important parameters to constrain the star formation history of galaxies. However, H ii regions…”
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The MUSE Ultra Deep Field (MUDF). VI. The Relationship between Galaxy Properties and Metals in the Circumgalactic Medium
Published in The Astrophysical journal (01-10-2024)“…Abstract We present initial results associating galaxies in the Multi-Unit Spectroscopic Explorer (MUSE) Ultra Deep Field (MUDF) with gas seen in absorption…”
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MUSE–ALMA Haloes – IX. Morphologies and stellar properties of gas-rich galaxies
Published in Monthly notices of the Royal Astronomical Society (29-07-2023)“…ABSTRACT Understanding how galaxies interact with the circumgalactic medium (CGM) requires determining how galaxies’ morphological and stellar properties…”
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Observational signatures of a warped disk associated with cold-flow accretion
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract We present MUSE observations of the field of the quasar Q0152−020, whose spectrum shows a Lyman limit system (LLS) at redshift zabs = 0.38, with a…”
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MUSE-ALMA haloes VI: coupling atomic, ionized, and molecular gas kinematics of galaxies
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT We present results of MUSE-ALMA haloes, an ongoing study of the circumgalactic medium (CGM) of galaxies (z ≤ 1.4). Using multiphase observations we…”
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Multiphase circumgalactic medium probed with MUSE and ALMA
Published in Monthly notices of the Royal Astronomical Society (11-05-2019)“…ABSTRACT Galaxy haloes appear to be missing a large fraction of their baryons, most probably hiding in the circumgalactic medium (CGM), a diffuse component…”
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The Baryonic Content of Galaxies Mapped by MaNGA and the Gas Around Them
Published in The Astrophysical journal (01-09-2023)“…Abstract We analyze the cool gas in and around 14 nearby galaxies (at z < 0.1) mapped with the Sloan Digital Sky Survey IV MaNGA survey by measuring absorption…”
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Discovery of Super-enriched Gas ∼1 Gyr after the Big Bang
Published in Astrophysical journal. Letters (01-09-2023)“…Abstract Abundances of chemical elements in the interstellar and circumgalactic media of high-redshift galaxies offer important constraints on the…”
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