课题基金 / 基金详情

Resolution of structure and formation of galaxies by using highly precise astrometric observations

Resolution of structure and formation of galaxies by using highly precise astrometric observations
通过使用高精度天体测量观测来解析星系的结构和形成
批准号:
13640249
负责人:
GOUDA naoteru
金额:
$1.15万
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
2001
资助国家:
日本
项目状态:
已结题
起止时间:
2001 至 2002

项目摘要

项目成果

相似基金

相关文献

中文摘要
翻译
我们研究了以下与银河系动力结构有关的理论分析,并密切关注未来高精度的天体测量观测结果。此外,还进行了红外天文测量卫星计划。旋臂的起源:虽然密度波理论是解释旋臂起源的一个很好的候选理论,但它的真伪尚不确定。我们提出了一种利用高精度天文观测所获得的恒星运动学信息来确定密度波是否是起源的方法。此外,我们还发现一个俯仰角可以由杆势影响的平衡和螺旋臂的形状来决定。由于视差对距离的改变,视差误差较大时,会产生一些偏差,因此需要注意。然后我们开发了一种不会产生偏差的新方法。3 .动力学结构模型的建立:研究了建立银河系动力学结构理论模型的方法。我们用半解析的方法分析了宇宙早期星系的形成和演化,以及可能与星系演化密切相关的QSO。对红外天文测量卫星方案进行了研究。对原始规范进行了总结。
英文摘要
We examined the following theoretical analyses in connection with the dynamical structure of the Galaxy, keeping an eye on the highly precise astrometric observations coming out in the future. Furthermore the infrared astrometry satellite plan itself was performed.1. The origin of the Spiral arms : although the density wave theory is a good candidate which can explain the origin of spiral arms , it is not sure whether it is true or not. We developed a method which can determine whether the density wave is the origin or not by using the information on kinematics of stars which will be taken by high precise astrometric observations. Furthermore we found that a pitch angle might be decided by balance of the influence by bar potential, and pattern of a spiral arm.2. Since some biases arise when the error of a parallax is large in changing a parallax to a distance, cautions are required. Then we developed a new method which cannot produce biases.3. Construction of the model of dynamical structure : the method to construct theoretical models of the dynamical structure of the Galaxy was investigated.4. We analyzed formation and evolution of galaxies in the early stages of the universe, and moreover QSO which might be closely connected with evolutions of galaxies using the semi- analytical method.5. The infrared astrometry satellite plan was examined. The primitive specification was summarized.
期刊论文(17)
专著(0)
科研奖励(0)
会议论文
Nagashima, M. et al.: "Galaxy Number Counts in the Subaru Deep Field : Multiband Analysis in a Hierarchical Galaxy Formation Model"The Astrophysical Journal. 578. 675-688 (2002)
Nagashima, M. 等人:“Subaru 深场中的星系数量计数:分层星系形成模型中的多波段分析”《天体物理学杂志》。
DOI: --
发表时间:
期刊:
影响因子: --
作者: []
通讯作者:
16
    海外基金