Dynamical processes in stellar astrophysics: A combination of spectroscopic monitoring with state-of-the-art theoretical modeling

自2013年以来，来自汉堡天文台和瓜纳华托大学的天文学家一直在共同操作TIGRE设施，这是一个机器人和光谱望远镜，致力于研究长期监测各种类型的恒星，与理论专家密切合作进行大气建模和演化模型。这两个研究所之间的合作非常富有成果，已经在天体物理学的各个不同领域出版了各种出版物。为了响应德国研究基金会（DFG，德国研究基金会）和墨西哥国家科学技术理事会（CONACYT）于2016年7月发出的建议，为德墨联合研究项目提供资金，我们寻求财政支持，以继续我们成功的德墨合作。我们特别要求支持旅行和出版费用，以奋进解决以下科学问题：色球活动水平和旋转周期：超越威尔逊山样本恒星活动周期和发电机模式跨越HRD巨星的恒星活动特性时域数据的统计分析极高-目标星分辨光谱学PHOENIX和演化模型对TIGRE目标的定量诊断现象和奇异物体

Since 2013 astronomers from Hamburg Observatory and the Universidad de Guanajuato have together been operating the TIGRE facility, a robotic and spectroscopic telescope dedicated to the study of long-term monitoring of various types of stars, working in close collaboration with theoretical experts for atmospheric modeling and evolution models. The collaboration between the two institutes has been extremely fruitful and has already resulted in a variety of publications in a variety of different fields in astrophysics. In response to the call for proposals issued by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) and the Mexican National Council for Science and Technology (CONACYT) in July 2016 to fund joint German-Mexican research projects we seek financial support to continue our successful German-Mexican collaboration. We specifically ask for support for travel and publication costs in our endeavor to tackle the following scientific issues:Chromospheric activity level and rotation periods: Beyond the Mount Wilson sampleStellar activity periods and dynamo modes across the HRDStellar activity properties of giantsStatistical analysis of time domain dataExtremely high-resolution spectroscopy of target starsQuantitative diagnostics of TIGRE targets by PHOENIX and evolution modelsBinary stars with phase dependent phenomena and exotic objects