Add to ORKGWe present analytical expressions for direct evaluation of ℓ-mixing rate coefficients in proton-excited hydrogen atom collisions and describe a software package for efficient numerical evaluation of the collisional rate coefficients. Comparisons between rate coefficients calculated with various levels of approximation are discussed, highlighting their range of validity. These rate coefficients are benchmarked for radio recombination lines for hydrogen, evaluating the corresponding departure coefficients from local thermal equilibrium
Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization bala...
Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization bala...
Hydrogen and helium emission lines in nebulae form by radiative recombination. This is a simple proc...
Precise spectral diagnostic modelling of H i and He ii recombination spectra can constrain theoretic...
Rate coefficients for rotational transitions in H2 induced by H2 impact are presented. Extensive qua...
Free-access link :https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stac3221/6815741?...
The recent detection of anions in the interstellar medium has shown that they exist in a variety of ...
We present calculated rate coefficients for ro-vibrational transitions of CO in collisions with H at...
Our knowledge about the cold universe often relies on molecular spectra. A general property of such ...
Hydronium (H3O+) was first detected in 1986 in interstellar molecular clouds. It was reported in man...
We have computed the rate of collisional cooling of a gas by H2 molecules under conditions appropria...
We present analytic fits to charge exchange rate coefficients over the full range of temperatures wh...
Hydrogen and helium emission lines in nebulae form by radiative recombination. This is a simple proc...
Cosmological models can be constrained by determining primordial abundances. Accurate predictions of...
Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization bala...
Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization bala...
Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization bala...
Hydrogen and helium emission lines in nebulae form by radiative recombination. This is a simple proc...
Precise spectral diagnostic modelling of H i and He ii recombination spectra can constrain theoretic...
Rate coefficients for rotational transitions in H2 induced by H2 impact are presented. Extensive qua...
Free-access link :https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stac3221/6815741?...
The recent detection of anions in the interstellar medium has shown that they exist in a variety of ...
We present calculated rate coefficients for ro-vibrational transitions of CO in collisions with H at...
Our knowledge about the cold universe often relies on molecular spectra. A general property of such ...
Hydronium (H3O+) was first detected in 1986 in interstellar molecular clouds. It was reported in man...
We have computed the rate of collisional cooling of a gas by H2 molecules under conditions appropria...
We present analytic fits to charge exchange rate coefficients over the full range of temperatures wh...
Hydrogen and helium emission lines in nebulae form by radiative recombination. This is a simple proc...
Cosmological models can be constrained by determining primordial abundances. Accurate predictions of...
Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization bala...
Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization bala...
Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate ionization bala...
Hydrogen and helium emission lines in nebulae form by radiative recombination. This is a simple proc...