Data Service: TEUV
Description
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.
This section describes who is responsible for this resource
Publisher: The GAVO DC team
Contact Information:
This section provides some status information: the resource version, availability, and relevant dates.
This resource was registered on: 2013 Feb 01 14:00:00ZThis resource description was last updated on: 2024 Dec 27 08:31:04Z
This section describes what the resource is, what it contains, and how it might be relevant.
This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
This NAVO Application is hosted by the Space Telescope Science Institute