The Origin of Da Scaling: Suppressed Cooling in Fast-cooling Mixing Layers
In numerical experiments simulating turbulent radiative mixing layers (TRMLs), it is observed that as the cooling time in the mixed gas, t _cool , becomes very short compared to the dynamical time of the turbulence, t _eddy / t _cool ≫ 1, there is a ...
Lachlan Lancaster +3 more
doaj +1 more source
Turbulence in the Local Interstellar Medium and the <i>IBEX</i> Ribbon. [PDF]
Zirnstein EJ +5 more
europepmc +1 more source
Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium. [PDF]
Zhou J +17 more
europepmc +1 more source
Computational prediction for the formation of amides and thioamides in the gas phase interstellar medium. [PDF]
Akbar Ali M, Thripati S.
europepmc +1 more source
More π, please: What drives the formation of unsaturated molecules in the interstellar medium? [PDF]
Londoño-Restrepo J +4 more
europepmc +1 more source
On the formation of 2- and 3-cyanofurans and their protonated forms in interstellar medium conditions: quantum chemical evidence. [PDF]
Simbizi R +4 more
europepmc +1 more source
Low-temperature gas-phase formation of cyclopentadiene and its role in the formation of aromatics in the interstellar medium. [PDF]
Yang Z +6 more
europepmc +1 more source
A possible direct exposure of the Earth to the cold dense interstellar medium 2-3 Myr ago. [PDF]
Opher M, Loeb A, Peek JEG.
europepmc +1 more source
A Vision for the Future of Astrochemistry in the Interstellar Medium by 2050. [PDF]
Fortenberry RC.
europepmc +1 more source

