Information on Service 'TEUV'
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:
-
external --
a renderer with some custom access method that should be mentioned in the service description
This service is published as follows:
- Within the
set(s) ivo_managed with the renderer
external
local means it is listed on our front page,
ivo_managed means
it has a record in the VO registry.
Citation Info
VOResource XML (that's something exclusively for VO nerds)