206 citations · 1.8k across the 61 of their papers we have counts for
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Gas kinematics around filamentary structures in the Orion B cloud
Mathilde Gaudel, Jan H. Orkisz, Maryvonne Gerin +27
Understanding the initial properties of star-forming material and how they affect the star formation process is key. From an observational point of view, the feedback from young hi…
Efficient sampling of non log-concave posterior distributions with mixture of noises
Pierre Palud, Pierre-Antoine Thouvenin, Pierre Chainais +2
This paper focuses on a challenging class of inverse problems that is often encountered in applications. The forward model is a complex non-linear black-box, potentially non-inject…
OH mid-infrared emission as a diagnostic of HO UV photodissociation. II. Application to interstellar PDRs
Marion Zannese, Benoît Tabone, Emilie Habart +3
Water photodissociation in the 114 - 144 nm UV range forms excited OH which emits at mid-infrared wavelengths via highly excited rotational lines. These lines have only been detect…
High angular resolution near-IR view of the Orion Bar revealed by Keck/NIRC2
Emilie Habart, Romane Le Gal, Carlos Alvarez +7
Nearby Photo-Dissociation Regions (PDRs), where the gas and dust are heated by the far UV-irradiation emitted from stars, are ideal templates to study the main stellar feedback pro…
PDRs4All: A JWST Early Release Science Program on radiative feedback from massive stars
Olivier Berné, Émilie Habart, Els Peeters +134
Massive stars disrupt their natal molecular cloud material through radiative and mechanical feedback processes. These processes have profound effects on the evolution of interstell…