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Origin of CH+ in diffuse molecular clouds warm H2 and ion-neutral drift
Valeska Valdivia, Benjamin Godard, Patrick Hennebelle +3
This paper assesses the roles of the presence of warm H2, and the increased formation rate due to the ion-neutral drift. We performed ideal MHD simulations that include the heating…
Tracing extended low-velocity shocks through SiO emission - Case study of the W43-MM1 ridge
F. Louvet, F. Motte. A. Gusdorf, Q. Nguyen-Luong +7
Previous literature suggests that the densest structures in the interstellar medium form through colliding flows, but patent evidence of this process is still missing. Recent liter…
Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. I. N159W
Min-Young Lee, Suzanne Madden, Vianney Lebouteiller +25
We present Herschel SPIRE Fourier Transform Spectrometer (FTS) observations of N159W, an active star-forming region in the Large Magellanic Cloud (LMC). In our observations, a numb…
3D radiative hydrodynamic simulations of protostellar collapse with H-C-O dynamical chemistry
Natalia Dzyurkevich, Benoît Commerçon, Pierre Lesaffre +1
Combining the co-evolving chemistry, hydrodynamics and radiative transfer is an important step for star formation studies. It allows both a better link to observations and a self-c…