Dust Evolution and the Formation of Planetesimals
文献类型：期刊论文
| 作者 | Birnstiel, T.1,2; Fang, M.3,4 ; Johansen, A.5
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| 刊名 | SPACE SCIENCE REVIEWS
 |
| 出版日期 | 2016-12-01 |
| 卷号 | 205期号:1-4页码:41-75 |
| ISSN号 | 0038-6308 |
| 关键词 | Accretion disks Planets and satellites: formation Protoplanetary disks Circumstellar matter |
| DOI | 10.1007/s11214-016-0256-1 |
| 通讯作者 | Birnstiel, T.(tbirnstiel@cfa.harvard.edu) |
| 英文摘要 | The solid content of circumstellar disks is inherited from the interstellar medium: dust particles of at most a micrometer in size. Protoplanetary disks are the environment where these dust grains need to grow at least 13 orders of magnitude in size. Our understanding of this growth process is far from complete, with different physics seemingly posing obstacles to this growth at various stages. Yet, the ubiquity of planets in our galaxy suggests that planet formation is a robust mechanism. This chapter focuses on the earliest stages of planet formation, the growth of small dust grains towards the gravitationally bound "planetesimals", the building blocks of planets. We will introduce some of the key physics involved in the growth processes and discuss how they are expected to shape the global behavior of the solid content of disks. We will consider possible pathways towards the formation of larger bodies and conclude by reviewing some of the recent observational advances in the field. |
| WOS关键词 | YOUNG STELLAR OBJECTS ; T-TAURI STARS ; SPECTRAL ENERGY-DISTRIBUTIONS ; SPITZER-SPACE-TELESCOPE ; MAIN-SEQUENCE STARS ; TRANSITIONAL PROTOPLANETARY DISKS ; HIGH-RESOLUTION SUBMILLIMETER ; POLARIZED SCATTERED-LIGHT ; HEAD-ON COLLISIONS ; HERBIG AE/BE STARS |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | SPRINGER |
| WOS记录号 | WOS:000391769100003 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/23348]  |
| 专题 | 中国科学院紫金山天文台 |
| 通讯作者 | Birnstiel, T. |
| 作者单位 | 1.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA 2.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany 3.Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Peoples R China 4.Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Peoples R China 5.Lund Univ, Lund Observ, Dept Astron & Theoret Phys, Box 43, S-22100 Lund, Sweden |
| 推荐引用方式 GB/T 7714 | Birnstiel, T.,Fang, M.,Johansen, A.. Dust Evolution and the Formation of Planetesimals[J]. SPACE SCIENCE REVIEWS,2016,205(1-4):41-75. |
| APA | Birnstiel, T.,Fang, M.,&Johansen, A..(2016).Dust Evolution and the Formation of Planetesimals.SPACE SCIENCE REVIEWS,205(1-4),41-75. |
| MLA | Birnstiel, T.,et al."Dust Evolution and the Formation of Planetesimals".SPACE SCIENCE REVIEWS 205.1-4(2016):41-75. |
入库方式： OAI收割
来源：紫金山天文台
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