Identification of the 4486,4504A emission lines in O-type spectra
Astrophysics
2007-05-23 v1
Abstract
Inspired by an appeal to the community from Walborn (these proceedings) we decided to solve the long-standing problem concerning the nature of the 4486,4504A emission lines, which are frequently observed in O-type spectra and which are particularly prominent in supergiants. We claim that these lines emerge from sulfur, namely by de-excitation of a highly excited S IV doublet state. We prove this by an exploratory NLTE calculation with a detailed model atom.
Keywords
Cite
@article{arxiv.astro-ph/0102006,
title = {Identification of the 4486,4504A emission lines in O-type spectra},
author = {K. Werner and T. Rauch},
journal= {arXiv preprint arXiv:astro-ph/0102006},
year = {2007}
}
Comments
4 pages, 3 figures. To appear in: Eta Carinae and Other Mysterious Stars, ASP Conference Series, Vol. xxx, 2001, T. Gull, S. Johansson, and K. Davidson, eds