Information on Service 'TEUV'

[Use this service from your browser]

Further access options are discussed below

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.

For a list of all services and tables belonging to this service's resource, see Information on resource 'TEUV'

Overview

You can access this service using:

This service is published as follows:

local means it is listed on our front page, ivo_managed means it has a record in the VO registry.

VOResource XML (that's something exclusively for VO nerds)