A Grid of Synthetic Stellar UV Fluxes
Abstract
We present preliminary results of a large project aimed at creating an extended theoretical and observational database of stellar spectra in the ultraviolet wavelength range. This library will consist of IUE spectra at low and high resolution, and a set of LTE and NLTE theoretical fluxes. A first grid of 50 model fluxes with solar metallicity, in the wavelength interval 1000 - 4400 AA, is reported here. Calculations are based on the Kurucz (1993) SYNTHE code. The models span effective temperatures between 10,000 K and 50,000 K, and a surface gravity in the range 2.5 <= log g <= 5.0 dex.
Cite
@article{arxiv.astro-ph/0107285,
title = {A Grid of Synthetic Stellar UV Fluxes},
author = {Lino H. Rodriguez-Merino and Miguel Chavez and Alberto Buzzoni and Emanuele Bertone},
journal= {arXiv preprint arXiv:astro-ph/0107285},
year = {2016}
}
Comments
2 pages, 1 figure, To appear in proceedings, "New Quests in Stellar Astrophysics: The Link Between Stars and Cosmology ", March 26-30, 2001, Eds. M. Chavez, A. Bressan, A. Buzzoni & D. Mayya