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.
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Tables defined within this resource descriptor
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