Probing Circumstellar Disk Properties with Polarization

几乎所有新形成的恒星周围的星周盘都是行星的诞生地，而盘内的物理条件决定了行星的形成。该项目将使用来自阿塔卡马大型毫米/亚毫米阵列（阿尔马）的高质量偏振观测来详细研究附近的星周盘。 由于偏振机制强烈依赖于波长，偏振观测是探测星周盘内部亚结构和磁场的敏感手段。 使用偏振模型，研究人员将探索磁盘偏振和从它推断的属性如何随着时间的推移而演变。 该项目的成果将促进天文学家对星星和行星形成的理解。 该项目将对一名研究生进行高级天文学技术和应用培训，为一名本科生提供研究经验，并对一个美洲土著部落进行科学宣传，研究小组将利用阿尔马进行偏振观测，以测量星周盘的性质，并将其置于系外行星探测的范围内。 该研究计划旨在：（1）解决通过偏振散射测量的最大尘埃颗粒尺寸之间的差异（~75微米）和从光谱指数推断的（~毫米）;（2）表征所观察到的偏振形态和强度随光源的波长的差异;（3）测量年轻圆盘的放大样品中的偏振，以将它们的性质与较老的金牛座T圆盘进行比较;以及（4）探测磁盘磁场或对其施加严格的观测约束。该奖项反映了NSF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。

Circumstellar disks surrounding nearly all newly formed stars are the birthplaces of planets, and the physical conditions within the disks govern the formation of planets. This project will use high quality polarization observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to study nearby circumstellar disks in detail. Because polarization mechanisms depend strongly on wavelength, polarization observations are a sensitive means to probe the substructures and magnetic fields within circumstellar disks. Using polarization models, the investigators will explore how disk polarization and the properties inferred from it evolve over time. Results from this project will advance astronomers’ understanding of star and planet formation. The project will train a graduate student in advanced astronomical techniques and applications, provide research experience to an undergraduate student, and conduct science outreach to a Native American tribe.The research team will undertake polarization observations using ALMA to measure the properties of circumstellar disks, placing them within the context of exoplanet detections. The research program seeks to: (1) address the discrepancy between maximum dust grain sizes measured by polarization scattering (~75 micron) and ones inferred from spectral indices (~millimeter); (2) characterize the differences in observed polarization morphology and intensity with wavelength for a large sample of sources; (3) measure polarization in an enlarged sample of young disks to compare their properties to the older T Tauri disks; and (4) detect disk magnetic fields or place stringent observational constraints on them.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.