Information on resource 'TEUV'

TEUV corrects synthetic stellar fluxes for interstellar absorption for wavelengths smaller than 91.1 nm. It simulates radiative bound-free absorption of the ground states of H, He, C, N, and O using Opacity Project data. Two interstellar components with different radial and turbulent velocities, temperatures, and column densities are considered.

Services defined within this resource descriptor

[Manage RD]