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Probing Galactic Structure and Evolution with Extragalactic Planetary Nebulae

Probing Galactic Structure and Evolution with Extragalactic Planetary Nebulae
用河外行星状星云探测银河系结构和演化
批准号:
0607416
负责人:
Robin Ciardullo
金额:
$22.95万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2006
资助国家:
美国
项目状态:
已结题
起止时间:
2006-08-01 至 2011-07-31

项目摘要

项目成果

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中文摘要
翻译
宾夕法尼亚州立大学:Robin CiardulloTitle:利用河外行星星云探测银河系结构和演化宾夕法尼亚州立大学的Robin Ciardullo将承担三个利用河外行星星云(PNE)来研究天体物理问题的项目。这些项目包括:1)测量PNE在近面对面螺旋线上的垂直运动学,以限制星系盘质量;2)测量M31星系凸起中PNE的组成,以了解明显的低氧丰度,并确定IA型超新星在M31凸起演化中的作用;3)探索室女座星系团内PNE的运动学,确定星系团内恒星在星系团内的相对重要性。这项工作产生的更广泛影响的主要领域涉及本科生和研究生的培训,重点是来自传统上代表不足的群体的学生。河外行星星云有如此多的用途,这一事实表明,从事这一项目的学生接触到了大量的天文学主题。最后,还将开展公众宣传活动。
英文摘要
AST-0607416INSTITUTION: Pennsylvania State UniversityPI: Robin CiardulloTITLE: Probing Galactic Structure and Evolution with Extragalactic Planetary NebulaeABSTRACTDr.. Robin Ciardullo, at the Pennsylvania State University, will undertake three projects that utilize extragalactic planetary nebulae (PNe) to investigate astrophysical questions. The projects consist of: 1) the measurement of the perpendicular kinematics of PNe in near face-on spirals, to constrain galaxy disk masses; 2) the measurement of the composition of PNe in the bulge of the galaxy M31, to understand both an apparent low oxygen abundance and to determine the role of type IA supernovae in the evolution of the M31 bulge; and 3) to probe the kinematics of the Virgo cluster intra-cluster PNe, to determine the relative importance of intra-cluster stars within cluster galaxies..The major area of broader impact that results from this work involves the training of undergraduate and graduate students, with an emphasis on students from traditionally under-represented groups. The fact that extragalactic planetary nebulae have so many uses suggests that students who work on this project are exposed to a great many topics in astronomy. Finally, public outreach activities will also be undertaken.
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会议论文
Integral Field Spectroscopy and the Hubble Constant
Collaborative Research: Galaxy Growth in Different Environments in the Early Universe from z=1.9 to 3.5
Probing the Evolution of Galaxies and Clusters with Planetary Nebulae
Measuring Distances and Stellar Kinematics with Extragalactic Planetary Nebulae
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