Search Results - "Jacques Le Bourlot"
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Learning from model grids: Tracers of the ionization fraction in the ISM
Published in EPJ Web of Conferences (2022)“…The ionization fraction in neutral interstellar clouds is a key physical parameter controlling multiple physical and chemical processes, and varying by orders…”
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Understanding the temperatures of H3 + and H2 in diffuse interstellar sightlines
Published in Molecular physics (17-01-2024)“…The triatomic hydrogen ion $ \mathrm {H}_3^+ $ H 3 + is one of the most important species for the gas phase chemistry of the interstellar medium. Observations…”
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Revealing which Combinations of Molecular Lines are Sensitive to the Gas Physical Parameters of Molecular Clouds
Published in EPJ Web of Conferences (01-01-2022)“…Atoms and molecules have long been thought to be versatile tracers of the cold neutral gas in the universe, from high-redshift galaxies to star forming regions…”
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H I-TO-H 2 TRANSITIONS AND H I COLUMN DENSITIES IN GALAXY STAR-FORMING REGIONS
Published in The Astrophysical journal (20-07-2014)Get full text
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A highly efficient Voigt program for line profile computation
Published in Journal of quantitative spectroscopy & radiative transfer (01-01-2025)“…Evaluation of the Voigt function, a convolution of a Lorentzian and a Gaussian profile, is essential in various fields such as spectroscopy, atmospheric…”
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Sustained oscillations in Interstellar chemistry models
Published 22-10-2020“…A&A 643, A121 (2020) Non-linear behavior in interstellar chemical models has been recognized for 25 years now. Different mechanisms account for the possibility…”
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Quantifying the informativity of emission lines to infer physical conditions in giant molecular clouds. I. Application to model predictions
Published 21-09-2024“…A&A 691, A109 (2024) Observations of ionic, atomic, or molecular lines are performed to improve our understanding of the interstellar medium (ISM). However,…”
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Neural network-based emulation of interstellar medium models
Published 04-09-2023“…A&A 678, A198 (2023) The interpretation of observations of atomic and molecular tracers in the galactic and extragalactic interstellar medium (ISM) requires…”
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Understanding the temperatures of H 3 + and H 2 in diffuse interstellar sightlines
Published in Molecular physics (17-01-2024)Get full text
Journal Article -
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Deep learning denoising by dimension reduction: Application to the ORION-B line cubes
Published 24-07-2023“…A&A 677, A158 (2023) Context. The availability of large bandwidth receivers for millimeter radio telescopes allows the acquisition of…”
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Journal Article -
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Gas kinematics around filamentary structures in the Orion B cloud
Published 25-11-2022“…A&A 670, A59 (2023) Understanding the initial properties of star-forming material and how they affect the star formation process is key. From an observational…”
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The chemistry of disks around T Tauri and Herbig Ae/Be stars
Published 26-03-2018“…A&A 616, A19 (2018) Infrared and (sub-)mm observations of disks around T Tauri and Herbig Ae/Be stars point to a chemical differentiation between both types of…”
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A Model for Atomic and Molecular Interstellar Gas: The Meudon PDR Code
Published in The Astrophysical journal (01-06-2006)“…We present the revised ``Meudon'' model of photon-dominated region (PDR) code, available on the Web under the GNU Public License. General organization of the…”
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Chemical Evolution of Turbulent Multiphase Molecular Clouds
Published 06-11-2017“…Molecular clouds are essentially made up of atomic and molecular hydrogen, which in spite of being the simplest molecule in the ISM plays a key role in the…”
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Journal Article -
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Chemical modeling of internal photon-dominated regions surrounding deeply embedded HC/UCHII regions
Published 22-03-2018“…A&A 617, A60 (2018) We aim to investigate the chemistry of internal photon-dominated regions surrounding deeply embedded hypercompact and ultracompact HII…”
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Origin of CH+ in diffuse molecular clouds warm H2 and ion-neutral drift
Published 16-12-2016“…A&A 600, A114 (2017) This paper assesses the roles of the presence of warm H2, and the increased formation rate due to the ion-neutral drift. We performed…”
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Tracers of the ionization fraction in dense and translucent gas: I. Automated exploitation of massive astrochemical model grids
Published 27-07-2020“…A&A 645, A28 (2021) The ionization fraction plays a key role in the physics and chemistry of the neutral interstellar medium, from controlling the coupling of…”
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C18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud: An analysis of the precision achievable when modeling spectral line within the Local Thermodynamic Equilibrium approximation
Published 17-05-2020“…A&A 645, A26 (2021) CO isotopologue transitions are routinely observed in molecular clouds to probe the column density of the gas, the elemental ratios of…”
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Journal Article -
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Efficient ortho-para conversion of H2 on interstellar grain surfaces
Published 17-01-2016“…A&A 588, A27 (2016) Context: Fast surface conversion between ortho- and para-H2 has been observed in laboratory studies, and this mechanism has been proposed…”
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Journal Article -
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A Fully Bayesian Approach For Inferring Physical Properties With Credibility Intervals From Noisy Astronomical Data
Published in 10th Workshop on Hyperspectral Imaging and Signal Processing: Evolution in Remote Sensing (WHISPERS), Amsterdam, Netherlands (01-09-2019)“…The atoms and molecules of interstellar clouds emit photons when passing from an excited state to a lower energy state. The resulting emission lines can be…”
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Conference Proceeding