中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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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