工作组摘要-本地宇宙
Working Group Summary - Local Universe
摘要:
这是在致力于本地宇宙研究的工作组中进行的讨论的摘要。作者按字母顺序排列,在工作组组织者之后,是那些在克里特岛的一周中发表演讲的人;他们的贡献被纳入这里。在小组讨论期间,我们考虑了未来在光学/红外波长下对单个恒星和恒星形成区域的研究之间存在的各种协同作用,这些研究将可能与E-ELT以及ALMA和SKA在类似区域中的分子和中性气体有关。主要的重点是恒星的形成;无论是在大规模和小规模。新的设施将使我们能够更详细地了解我们自己的银河系的性质,也使我们能够与一系列更遥远的系统进行详细的比较,这些系统都是在不同的初始条件下以不同的速度形成恒星的(例如,金属丰度)和不同的空间分布。
英文摘要:
This is a summary of the discussions that took place in the working group dedicated to studies of the Local Universe. The authors are listed in alphabetical order, after the working group organiser, and are those who gave a presentation during the week in Crete; their contributions are incorporated here. During the group discussions we considered the various synergies that exist between future studies of individual stars and star formation regions at optical/IR wavelengths that will be possible with the E-ELT and those of the molecular and neutral gas in similar regions that will be possible with ALMA and SKA. The primary emphasise was on star formation; both on large and small scales. New facilities will allow more detailed insights into the properties of our own Galaxy and also allow us to make detailed comparisons with a range of more distant systems all forming stars at different rates from different initial conditions (e.g., metallicity) and with different spatial distributions.
机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。