engleski

Lithium, sodium and potassium resonance lines pressure broadened by helium atoms .

The resonance lines of alkali-metal atoms, broadened by collisions with helium atoms, are prominent features in the spectra of brown dwarfs. We carried out calculations of the emission and absorption spectra in the far red and blue wings of the first resonant doublets of lithium, sodium and potassium perturbed by helium atoms, for temperatures from 500 to 3000 K. For our calculation we used carefully constructed electronic adiabatic potential energy curves and electronic transition dipole moments of Li-He, Na-He and K-He molecules. In the computation of the emission and absorption coefficients, we used the fully quantum- mechanical calculation, based on the Fourier grid Hamiltonian method. The obtained absorption and emission spectra are compared with previous theoretical calculations.

Molecular data - line: profiles - stars: brown dwarfs

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