| タイトル | B Stars with and without emission lines, parts 1 and 2 |
| 本文（外部サイト） | http://hdl.handle.net/2060/19820017151 |
| 著者（英） | Doazan, V.; Underhill, A. |
| 著者所属（英） | Centre National de la Recherche Scientifique; NASA Headquarters |
| 発行日 | 1982-01-01 |
| 言語 | eng |
| 内容記述 | The spectra for B stars for which emission lines occur not on the main sequence, but only among the supergiants, and those B stars for which the presence of emission in H ahlpa is considered to be a significant factor in delineating atmospheric structure are examined. The development of models that are compatible with all known facts about a star and with the laws of physics is also discussed. |
| NASA分類 | SPACE SCIENCES (GENERAL) |
| レポートNO | 82N25027
NASA-SP-456
NAS 1.21:456
LC-82-2313 |
| 権利 | No Copyright |
