| タイトル | Spectral energy distributions of T Tauri stars - Disk flaring and limits on accretion |
| 著者（英） | Kenyon, S. J.; Hartmann, L. |
| 著者所属（英） | Harvard-Smithsonian Center for Astrophysics |
| 発行日 | 1987-12-15 |
| 言語 | eng |
| 内容記述 | The Adams et al. (1987) conclusion that much of the IR excess emission in the spectral energy distribution of T Tauri stars arises from reprocessing of stellar radiation by a dusty circumstellar disk is presently supported by analyses conducted in light of various models of these stars' spectra. A low mass reprocessing disk can, however, produce these spectra as well as a massive accretion disk. The detection of possible boundary layer radiation in the optical and near-UV regions poses the strongest limits on accretion rates. Disk accretion in the T Tauri phase does not significantly modify stellar evolution. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 88A23602 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/372771 |
