9 citations · 26 across the 13 of their papers we have counts for
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Supernova Shocks in Molecular Clouds: Shocks Driven into Dense Cores in IC 443 and 3C 391
William T. Reach, Ngoc Le Tram, Curtis DeWitt +3
Supernova shocks into dense molecular cores in IC 443 (clumps B, C, and G) and 3C 391 were observed using the Stratospheric Observatory for Infrared Astronomy and complemented by a…
Physical conditions in Centaurus A's northern filaments II: Does the HCO emission highlight the presence of shocks?
Quentin Salomé, Philippe Salomé, Benjamin Godard +2
Abridged: We present the first observation of the HCO+(1-0) and HCN(1-0) emission in the northern filaments of Centaurus A with ALMA. HCO+(1-0) is detected in 9 clumps of the Horse…
The Molecular Cloud Lifecycle I: Constraining H2 formation and dissociation rates with observations
Shmuel Bialy, Blakesley Burkhart, Daniel Seifried +9
Molecular clouds (MCs) are the birthplaces of new stars in galaxies. A key component of MCs are photodissociation regions (PDRs), where far-ultraviolet radiation plays a crucial ro…
Shocks in the warm neutral medium II -- Origin of neutral carbon at high pressure
Benjamin Godard, Guillaume Pineau Des Forêts, Jeremy La Porte +1
Aims: Ultraviolet (UV) lines of neutral carbon observed in absorption in the local diffuse interstellar medium (ISM) have long revealed that a substantial fraction of the mass of t…
Radiative and mechanical energies in galaxies I. Contributions of molecular shocks and PDRs in 3C 326 N
J. A. Villa-Vélez, B. Godard, P. Guillard +1
Context: Atomic and molecular lines in galaxies offer insights into energy budgets and feedback mechanisms. Aims: This study establishes a new framework for interpreting these line…
Shocks in the warm neutral medium I -- Theoretical model
Benjamin Godard, Guillaume Pineau Des Forêts, Shmuel Bialy
Context. Atomic and molecular line emissions from shocks may provide valuable information on the injection of mechanical energy in the interstellar medium (ISM), the generation of…