Radiative transfer modeling of three T Tauri stars: selecting candidates for studying circumstellar disk evolution
文献类型:期刊论文
作者 | Liu, Yao1,2,3,4; Wang, Hong-Chi1,2; Wolf, Sebastian4; Madlener, David4 |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
出版日期 | 2013-07-01 |
卷号 | 13期号:7页码:841-848 |
ISSN号 | 1674-4527 |
关键词 | circumstellar matter planetary systems: protoplanetary disks radiative transfer |
通讯作者 | Liu, Y (reprint author), Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China. Email: yliu@pmo.ac.cn |
英文摘要 | We present modeling work on three young stellar objects that are promising targets for future high-resolution observations to investigate circumstellar disk evolution. The currently available data comprise the spectral energy distribution from optical to millimeter wavelengths which allow constraining the structure of the circumstellar disk using self-consistent radiative transfer models. The results suggest that the assumption of well-mixed dust and gas leads to overestimation of flux in the far-infrared. Observational and theoretical arguments suggest that an overall decrease in far-infrared excess can be explained by dust settling towards the midplane. A new disk model is hence employed to take the effect of dust sedimentation into account. The extended model satisfactorily reproduces all existing observations. The three targets studied here therefore deserve follow-up observations to reveal the evolutionary state of their protoplanetary disks. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | INFRARED SPECTROGRAPH SPECTRA ; HERBIG AE/BE STARS ; PROTOPLANETARY DISKS ; DUST EVOLUTION ; GRAIN-GROWTH ; DISTRIBUTIONS ; EXTINCTION ; APPEARANCE ; SYSTEMS ; AURIGA |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000320859600008 |
公开日期 | 2014-01-08 |
源URL | [http://libir.pmo.ac.cn/handle/332002/9840] |
专题 | 紫金山天文台_分子云与恒星形成研究团组 |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China 3.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China 4.Univ Kiel, Inst Theoret Phys & Astrophys, D-24118 Kiel, Germany |
推荐引用方式 GB/T 7714 | Liu, Yao,Wang, Hong-Chi,Wolf, Sebastian,et al. Radiative transfer modeling of three T Tauri stars: selecting candidates for studying circumstellar disk evolution[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2013,13(7):841-848. |
APA | Liu, Yao,Wang, Hong-Chi,Wolf, Sebastian,&Madlener, David.(2013).Radiative transfer modeling of three T Tauri stars: selecting candidates for studying circumstellar disk evolution.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,13(7),841-848. |
MLA | Liu, Yao,et al."Radiative transfer modeling of three T Tauri stars: selecting candidates for studying circumstellar disk evolution".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 13.7(2013):841-848. |
入库方式: OAI收割
来源:紫金山天文台
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