Time-dependent chemistry in 3D MHD simulations leads to H3+ abundances that, when analyzed under steady-state assumptions, imply CRIR values 2-5 times higher than the true input rate, with a median factor of ~3.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
Numerical model of fast electron energy loss in H2 finds 11% of energy to direct ro-vibrational excitation and 1.5-2 times higher yields for high-vibrational states via electronic cascading than earlier Monte Carlo calculations.
SKAO will enable detection of synchrotron emission from prestellar cores to probe their magnetic field properties in nearby star-forming regions.
citing papers explorer
-
The cosmic ray ionization rate from H3+ observations can be overestimated due to neglect of time-dependent chemistry
Time-dependent chemistry in 3D MHD simulations leads to H3+ abundances that, when analyzed under steady-state assumptions, imply CRIR values 2-5 times higher than the true input rate, with a median factor of ~3.
-
Numerical model of fast electron energy deposition in interstellar molecular gas
Numerical model of fast electron energy loss in H2 finds 11% of energy to direct ro-vibrational excitation and 1.5-2 times higher yields for high-vibrational states via electronic cascading than earlier Monte Carlo calculations.
-
Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds
SKAO will enable detection of synchrotron emission from prestellar cores to probe their magnetic field properties in nearby star-forming regions.