PG
Pierre Gratier
Université de Bordeaux, CNRS Délégation Aquitaine-Limousin, Institut de Radioastronomie Millimétrique
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena
Employment
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Université de Bordeaux Astronome-Adjoint2016 - Present
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CNRS Délégation Aquitaine-Limousin Post-Doc2013 - 2016
- 2011 - 2013
Education
- 2007 - 2010
Projects & Funding
Projects & funding information is unavailable.
Publications (96)
- Chemical diversity of dense cores in Orion B: The role of the environment Save
- Predicting CO and dust emission of star-forming galaxies Save
- Ice chemistry that can be unveiled with the JWST: SynthIceSpec, a synthetic spectrum generator to test spectral limits Save
- Chemical constraints on the dynamical evolution of the cold core L694 Save
- Predicting HCN, HCO+, multitransition CO, and dust emission of star-forming galaxies Save
- The 2024 KIDA network for interstellar chemistry Save
- Astrochemical models of interstellar ices: History matters Save
- Confirmation of the outflow in L1451-mm: SiO line and CH3OH maser detections Save
- Chemical compositions of five Planck cold clumps Save
- C18O, 13CO, and 12CO abundances and excitation temperatures in the Orion B molecular cloud. Analysis of the achievable precision in modeling spectral lines within the approximation of the local thermodynamic equilibrium Save
- Quantitative inference of the H2 column densities from 3 mm molecular emission: case study towards Orion B Save
- Tracers of the ionization fraction in dense and translucent gas. I. Automated exploitation of massive astrochemical model grids Save
- A Decade with VAMDC: Results and Ambitions Save
- Gas-grain model of carbon fractionation in dense molecular clouds Save
- Influence of galactic arm scale dynamics on the molecular composition of the cold and dense ISM III. Elemental depletion and shortcomings of the current physico-chemical models Save
- Revised mass-radius relationships for water-rich rocky planets more irradiated than the runaway greenhouse limit Save
- Rotation of molecular clouds in M 51 Save
- Abundances of sulphur molecules in the Horsehead nebula Save
- Influence of galactic arm scale dynamics on the molecular composition of the cold and dense ISM – II. Molecular oxygen abundance Save
- Oxygen fractionation in dense molecular clouds Save