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DOI10.1126/science.1101979
Disks around stars and the growth of planetary systems
Greaves J.S.
发表日期2005
ISSN0036-8075
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
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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).
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