The dynamics of rotating triaxial galaxies with massive black holes

具有大质量黑洞的旋转三轴星系的动力学

• 批准号: 0908346
• 负责人: Monica Valluri
• 金额: $ 44.01万
• 依托单位: Regents of the University of Michigan - Ann Arbor
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2009
• 资助国家: 美国
• 起止时间: 2009-09-01 至 2013-09-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0908346&HistoricalAwards=false
• 关键词: dynamics; rotating; triaxial; galaxies; massive

This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).Dr Valluri will study stellar motions in galaxies that are triaxial or have barred disks, and harbor supermassive black holes at their centers. Most elliptical galaxies are triaxial, and roughly half of all disk galaxies are barred. Despite this, the masses of their central black holes are generally determined by fitting axisymmetric (or even spherical) galaxy models to the observational data. Dr Valluri will start by investigating orbits in model triaxial potentials, finding the underlying frequencies of the regular orbits to classify them into their major families, and mapping out the regions where orbits are chaotic. She will then use the same technique on the orbits of particles in gravitational N-body simulations of rotating triaxial and barred galaxies, both with and without a central black hole. Finally, she will improve her current axisymmetric Schwarzschild code to include triaxiality and figure rotation. This code generates gravitationally self-consistent models that will be used to estimate the masses of the black holes at the centers of well-observed nearby galaxies. An undergraduate student will participate in the research. The anticipated results are of broad scientific interest, since mass estimates for galaxy-center black holes are used to constrain the efficiency with which active galactic nuclei radiate energy, and to estimate how often the merger of binary supermassive black holes should be detectable by gravitational wave experiments. Dr Valluri will lead a discussion and mentoring group for women graduate students and undergraduate students in her department. She will also carry out hands-on astronomy projects for K-12 students in collaboration with the University of Michigan's Museum of Natural History and Planetarium.

该奖项是根据2009年美国复苏和再投资法案（公法111-5）资助的。Valluri博士将研究三轴星系或有棒状圆盘的星系的恒星运动，这些星系的中心有超大质量黑洞。大多数椭圆星系是三轴的，大约一半的盘状星系是棒状的。尽管如此，它们中心黑洞的质量通常是通过将轴对称（甚至球形）星系模型拟合到观测数据中来确定的。Valluri博士将从研究模型三轴电位中的轨道开始，找到规则轨道的潜在频率，将它们分类到主要的家族中，并绘制出轨道混乱的区域。然后，她将使用相同的技术在旋转三轴星系和棒状星系的重力n体模拟中的粒子轨道上，无论有没有中心黑洞。最后，她将改进她目前的轴对称史瓦西代码，包括三轴性和图形旋转。该代码生成的引力自洽模型将用于估计在观测良好的附近星系中心的黑洞质量。一名本科生将参与研究。预期的结果具有广泛的科学意义，因为对星系中心黑洞的质量估计用于限制活动星系核辐射能量的效率，并用于估计通过引力波实验可以探测到双超大质量黑洞合并的频率。瓦卢里博士将在她的部门为女研究生和本科生领导一个讨论和指导小组。她还将与密歇根大学自然历史博物馆和天文馆合作，为K-12学生开展实践天文学项目。