| タイトル | Atomic Physics with the Goddard High-Resolution Spectrograph on the Hubble Space Telescope |
| 本文（外部サイト） | http://hdl.handle.net/2060/19970001813 |
| 著者（英） | Cardelli, Jason A.; Federman, S. R. |
| 著者所属（英） | Wisconsin Univ. |
| 発行日 | 1995-10-10 |
| 言語 | eng |
| 内容記述 | Interstellar spectra toward zeta Oph acquired with the Goddard High-Resolution Spectrograph were used to obtain oscillator strengths for approximately two dozen S I lines. This analysis was possible because precisely determined experimental oscillator strengths are available for several multiplets, including one with a weak interstellar line. The self-consistent set of oscillator strengths then was obtained from a curve of growth based on line strengths spanning a range of a factor of 100. The derived f-values for a number of multiplets differ from values quoted by Morton (1991) but are generally consistent with the suite of available experimental and theoretical results. |
| NASA分類 | Astronomy |
| レポートNO | 97N11582
NASA-CR-202492
NAS 1.26:202492 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
