| タイトル | Molecular Line and Continuum Opacities for Modeling of Extrasolar Giant Planet and Cool Stellar Atmospheres |
| 本文（外部サイト） | http://hdl.handle.net/2060/20030058932 |
| 著者（英） | Weck, P. F.; Hauschildt, P. H.; Allen, W. D.; Schweitzer, A.; Kirby, K.; Stancil, P. C.; Yamaguchi, Y. |
| 著者所属（英） | Georgia Univ. |
| 発行日 | 2002-11-01 |
| 言語 | eng |
| 内容記述 | The molecular line and continuum opacities are investigated in the atmospheres of cool stars and Extrasolar Giant Planets (EGPs). Using a combination of ab inito and experimentally derived potential curves and dipole transition moments, accurate data have been calculated for rovibrationally-resolved oscillator strengths and photodissociation cross sections in the B' (sup 2)Sigma+ (left arrow) X (sup 2)Sigma+ and A (sup 2)Pi (left arrow) X (sup 2)Sigma+ band systems in MgH. We also report our progress on the study of the electronic structure of LiCl and FeH. |
| NASA分類 | Astrophysics |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/565206 |
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