105 citations · 244 across the 4 of their papers we have counts for
4 papers
A dynamically young, gravitationally stable network of filaments in Orion B
Jan H. Orkisz, Nicolas Peretto, Jérôme Pety +15
Filaments are a key step on the path that leads from molecular clouds to star formation. However, their characteristics are heavily debated, and the exact processes that lead to th…
Stellar Feedback in the ISM Revealed by Wide-Field Far-Infrared Spectral-Imaging
Javier R. Goicoechea, Maryvonne Gerin, Emeric Bron
The radiative and mechanical interaction of stars with their environment drives the evolution of the ISM and of galaxies as a whole. The far-IR emission (lambda ~30 to 350 microns)…
Turbulence and star formation efficiency in molecular clouds: solenoidal versus compressive motions in Orion B
Jan H. Orkisz, Jérôme Pety, Maryvonne Gerin +13
The nature of turbulence in molecular clouds is one of the key parameters that control star formation efficiency: compressive motions, as opposed to solenoidal motions, can trigger…
Surface chemistry in the Interstellar Medium II. formation on dust with random temperature fluctuations
Emeric Bron, Jacques Le Bourlot, Franck Le Petit
The formation on grains is known to be sensitive to dust temperature, which is also known to fluctuate for small grain sizes due to photon absorption. We aim at expl…