Millimeter observations of the disk around GW Orionis
文献类型：期刊论文
| 作者 | Fang, M.1,2 ; Sicilia-Aguilar, A.1,3,4; Wilner, D.5; Wang, Y.6,7,8; Roccatagliata, V.9; Fedele, D.10; Wang, J. Z.11
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| 刊名 | ASTRONOMY & ASTROPHYSICS
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| 出版日期 | 2017-07-01 |
| 卷号 | 603页码:10 |
| 关键词 | circumstellar matter stars: pre-main sequence binaries: spectroscopic stars: individual: GW Orionis |
| ISSN号 | 1432-0746 |
| DOI | 10.1051/0004-6361/201628792 |
| 通讯作者 | Fang, M.(mfang.cn@gmail.com) |
| 英文摘要 | The GW Ori system is a pre-main sequence triple system (GW Ori A/B/C) with companions (GW Ori B/C) at similar to 1AU and similar to 8AU, respectively, from the primary (GW Ori A). The primary of the system has a mass of 3.9 M-circle dot, but shows a spectral type of G8. Thus, GW Ori A could be a precursor of a B star, but it is still at an earlier evolutionary stage than Herbig Be stars. GW Ori provides an ideal target for experiments and observations (being a "blown-up" solar system with a very massive sun and at least two upscaled planets). We present the first spatially resolved millimeter interferometric observations of the disk around the triple pre-main sequence system GW Ori, obtained with the Submillimeter Array, both in continuum and in the (CO)-C-12 J = 2-1, (CO)-C-13 J = 2 1, and (CO)-O-18 J = 2-1 lines. These new data reveal a huge, massive, and bright disk in the GW Ori system. The dust continuum emission suggests a disk radius of around 400AU, but the 12CO J = 2 1 emission shows a much more extended disk with a size around 1300AU. Owing to the spatial resolution (similar to 1"), we cannot detect the gap in the disk that is inferred from spectral energy distribution (SED) modeling. We characterize the dust and gas properties in the disk by comparing the observations with the predictions from the disk models with various parameters calculated with a Monte Carlo radiative transfer code RADMC-3D. The disk mass is around 0.12 M-circle dot, and the disk inclination with respect to the line of sight is around similar to 35 degrees. The kinematics in the disk traced by the CO line emission strongly suggest that the circumstellar material in the disk is in Keplerian rotation around GW Ori. Tentatively substantial (CO)-O-18 depletion in gas phase is required to explain the characteristics of the line emission from the disk. |
| WOS关键词 | MAIN-SEQUENCE STARS ; T-TAURI STARS ; ALL-SKY SURVEY ; FORMING REGIONS ; PROTOPLANETARY DISKS ; SUBMILLIMETER ARRAY ; PLANET FORMATION ; EVOLUTION ; DUST ; MULTIPLICITY |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000406619100013 |
| 出版者 | EDP SCIENCES S A |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/22649]  |
| 专题 | 中国科学院紫金山天文台 |
| 通讯作者 | Fang, M. |
| 作者单位 | 1.Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain 2.Univ Arizona, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA 3.Univ St Andrews, Sch Phys & Astron, SUPA, North Haugh, St Andrews KY16 9SS, Fife, Scotland 4.Univ Dundee, Sch Sci & Engn, Dundee DD1 4HN, Scotland 5.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA 6.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany 7.Chinese Acad Sci, Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China 8.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China 9.Ludwig Maximilians Univ Munchen, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany 10.INAF, Osservatorio Astrofis Arcetri, L Go E Fermi 5, I-50125 Florence, Italy |
| 推荐引用方式 GB/T 7714 | Fang, M.,Sicilia-Aguilar, A.,Wilner, D.,et al. Millimeter observations of the disk around GW Orionis[J]. ASTRONOMY & ASTROPHYSICS,2017,603:10. |
| APA | Fang, M..,Sicilia-Aguilar, A..,Wilner, D..,Wang, Y..,Roccatagliata, V..,...&Wang, J. Z..(2017).Millimeter observations of the disk around GW Orionis.ASTRONOMY & ASTROPHYSICS,603,10. |
| MLA | Fang, M.,et al."Millimeter observations of the disk around GW Orionis".ASTRONOMY & ASTROPHYSICS 603(2017):10. |
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来源：紫金山天文台
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