星團之形成與演化;Formation and Evolution of Star Clusters

NCU Institutional Repository > 理學院 > 天文研究所 > 研究計畫 > Item 987654321/62392

jsp.display-item.identifier=請使用永久網址來引用或連結此文件: http://ir.lib.ncu.edu.tw/handle/987654321/62392

题名:	星團之形成與演化;Formation and Evolution of Star Clusters
作者:	陳文屏
贡献者:	國立中央大學天文研究所
关键词:	物理
日期:	2012-12-01
上传时间:	2014-03-17 11:31:45 (UTC+8)
出版者:	行政院國家科學委員會
摘要:	研究期間：10101~10112;Most, and likely all, stars form out of collapsing molecular clouds in clustered environments. It has been known that low-mass stars outnumber massive stars, described as the initial mass function (IMF), in stellar systems from small star groups to clusters, to galaxies. The origin of a seemingly universal IMF is still largely unknown. Generally, massive stars are seen to concentrate near the center of a young star cluster, whereas lower-mass stars disperse in a larger volume. This effect of mass segregation is thought due partly to the original structure in the parental cloud and partly to the subsequent gravitational dynamics between member stars. We propose to strengthen the ongoing collaboration between the Taiwanese and Indian groups to conduct a systematic investigation of star clusters. Specifically, we will (1) conduct a search for uncharted star clusters by digital sky survey data such as 2MASS and Pan-STARRS. Low-mass members in known clusters will be identified. The comprehensive sample of Galactic open clusters will be a valuable tool not only for cluster evolution (mass segregation, stellar evaporation), but also for probing the formation and evolution of Galactic disk, (2) study a sample of open clusters in different Galactic environments to derive their IMFs, effect of mass segregation, and in particular, how massive stars influence the molecular clouds and induce the formation of nextgeneration stars.
關聯:	財團法人國家實驗研究院科技政策研究與資訊中心
显示于类别:	[天文研究所] 研究計畫

文件中的档案:

档案	描述	大小	格式	浏览次数
index.html		0Kb	HTML	373	检视/开启

在NCUIR中所有的数据项都受到原著作权保护.

社群 sharing

数据加载中.....