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.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/org.gavo.dc/gvo/data/teuv/teuv.iaat
Related Identifier http://dc.g-vo.org/gvo/data/teuv/teuv.iaat/info
Related Identifier http://astro.uni-tuebingen.de/~TEUV
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://org.gavo.dc/gvo/data/teuv/teuv.iaat
Provenance
Creator Müller-Ringat; E., Rauch, T.
Publisher The GAVO DC team
Publication Year 2013
OpenAccess true
Contact Thomas Rauch <astro-tmaw(at)listserv.uni-tuebingen.de>
Representation
Resource Type Dataset
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics