Climate Change Data Portal
DOI | 10.1126/science.1101979 |
Disks around stars and the growth of planetary systems | |
Greaves J.S. | |
发表日期 | 2005 |
ISSN | 0036-8075 |
起始页码 | 68 |
结束页码 | 71 |
卷号 | 307期号:5706 |
英文摘要 | Circumstellar disks play a vital evolutionary role, providing a way to move gas inward and onto a young star. The outward transfer of angular momentum allows the star to contract without breaking up, and the remnant disk of gas and particles is the reservoir for forming planets. High-resolution spectroscopy is uncovering planetary dynamics and motion within the remnant disk, and imaging at infrared to millimeter wavelengths resolves disk structure over billions of years of evolution. Most stars are born with a disk, and models of planet formation need to form such bodies from the disk material within the disk's 10-million-year life-span. |
英文关键词 | Disks (structural components); Gas dynamics; Spectroscopic analysis; Disk structure; High resolution spectroscopy; Planetary systems; Young stars; Planets; carbon; carbon monoxide; hydrogen; nitrogen; oxygen; astrophysics; astronomy; evolution; gas; infrared radiation; lifespan; mass spectrometry; motion; nuclear energy; priority journal; review; space flight; waveform |
语种 | 英语 |
来源期刊 | Science
![]() |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/243863 |
作者单位 | Physics and Astronomy, University of St. Andrews, North Haugh, St. Andrews, Fife KY16 9SS, United Kingdom |
推荐引用方式 GB/T 7714 | Greaves J.S.. Disks around stars and the growth of planetary systems[J],2005,307(5706). |
APA | Greaves J.S..(2005).Disks around stars and the growth of planetary systems.Science,307(5706). |
MLA | Greaves J.S.."Disks around stars and the growth of planetary systems".Science 307.5706(2005). |
条目包含的文件 | 条目无相关文件。 |
个性服务 |
推荐该条目 |
保存到收藏夹 |
导出为Endnote文件 |
谷歌学术 |
谷歌学术中相似的文章 |
[Greaves J.S.]的文章 |
百度学术 |
百度学术中相似的文章 |
[Greaves J.S.]的文章 |
必应学术 |
必应学术中相似的文章 |
[Greaves J.S.]的文章 |
相关权益政策 |
暂无数据 |
收藏/分享 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。