Collaborative Research: RUI: Protostellar jets across the mass spectrum

合作研究：RUI：跨质谱的原恒星喷流

• 批准号: 1910271
• 负责人: Dario Carbone
• 金额: $ 19.95万
• 依托单位: University of The Virgin Islands
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2019
• 资助国家: 美国
• 起止时间: 2019-09-01 至 2023-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1910271&HistoricalAwards=false
• 关键词: Collaborative; Research; RUI; Protostellar; jets

Stars, like our Sun, are known to form from clouds of molecular gas in interstellar space. These clouds gradually collapse under the influence of gravity, becoming denser and smaller. As this happens, any initial spin of the cloud is amplified, much like when an ice skater pulls their arms in to spin faster. This occurs because of a phenomenon known as the conservation of angular momentum. However, if material that was to form a star fully conserved its angular momentum, i.e., its degree of spin, then by the time it became as small as a star it would be spinning so quickly that it would no longer be stable and would be flung apart. The answer to this riddle of how stars like our Sun have been able to form, requiring quite low rates of spin, is thought to be related to the phenomenon of "Protostellar Jets", which is the subject of this research. Fast flowing gas, collimated into a pair of jets, is almost always seen when young stars are forming, i.e., when they are "protostars". These jets are thought to be launched from a spinning gas disk that surrounds the growing star because of the action of magnetic fields threading the disk that become wound up by the swirling gas. These magnetic fields are thought to become powerful enough to launch some of the gas from the disk, which carries away angular momentum from material left behind that can then eventually settle on to the star. The remnants of such disks may become systems of planets, like those of our solar system. The investigators seek to understand how stars and planets are born by better understanding how protostellar jets are launched. The investigators will perform computer simulations of protostellar jets understand their properties, including from relatively low-mass stars like our Sun, to much more massive stars that also exist in our Galaxy. The results of these simulations will be compared to observations of protostellar jets made by radio telescopes to test the theoretical simulations.The broader impact plan integrates research with teaching and public outreach activities. At the University of the Virgin Islands (UVI) three undergraduates will share in the research projects each year, providing important opportunities for STEM career development for underrepresented groups. This proposal will help strengthen a collaboration between this new research group at UVI and the University of Virginia (UVA). The collaboration plan includes student exchanges between UVI and UVA, expanding the horizons of both groups.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

恒星，比如我们的太阳，是由星际空间的分子气体云形成的。这些云在重力的影响下逐渐坍缩，变得越来越密，越来越小。当这种情况发生时，云的任何初始旋转都会被放大，就像溜冰者把手臂收起来旋转得更快一样。这是因为一种叫做角动量守恒的现象。然而，如果形成恒星的物质完全保持了它的角动量，也就是它的自旋程度，那么当它变得像恒星一样小的时候，它会旋转得太快，以至于它不再稳定，会被甩开。像我们的太阳这样的恒星是如何形成的，需要相当低的旋转速率，这个谜题的答案被认为与“原恒星喷流”现象有关，这是本研究的主题。当年轻的恒星形成时，即当它们是“原恒星”时，几乎总是可以看到快速流动的气体，它们被对准成一对射流。这些喷流被认为是从围绕着这颗正在成长的恒星的旋转气体盘发射出来的，因为磁场的作用穿过了被旋转气体缠绕的圆盘。这些磁场被认为变得足够强大，可以从圆盘上发射出一些气体，这些气体带走了残留物质的角动量，最终会落在恒星上。这些圆盘的残余物可能会变成行星系统，就像我们的太阳系一样。研究人员试图通过更好地了解原恒星喷流是如何发射的，来了解恒星和行星是如何诞生的。研究人员将对原恒星喷流进行计算机模拟，了解它们的特性，包括从质量相对较低的恒星（如我们的太阳）到同样存在于我们银河系中的大得多的恒星。这些模拟的结果将与射电望远镜观测到的原恒星喷流进行比较，以验证理论模拟。更广泛的影响计划将研究与教学和公共宣传活动结合起来。在维尔京群岛大学（UVI），每年将有三名本科生参与研究项目，为代表性不足的群体提供STEM职业发展的重要机会。这项提议将有助于加强弗吉尼亚大学这个新研究小组和弗吉尼亚大学（UVA）之间的合作。该合作计划包括UVI和UVA之间的学生交换，扩大双方的视野。该奖项反映了美国国家科学基金会的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。