High-resolution, mid-infrared spectroscopy of young stellar environments

年轻恒星环境的高分辨率中红外光谱

• 批准号: 0708074
• 负责人: Matthew Richter
• 金额: $ 47.15万
• 依托单位: University of California-Davis
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2007
• 资助国家: 美国
• 起止时间: 2007-08-15 至 2011-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0708074&HistoricalAwards=false
• 关键词: resolution; mid; infrared; spectroscopy; young

This project will utilize the unique observational technology developed in part by Dr. Richter to advance our understanding of the origin of planets. Using the Texas Echelon-cross-Echelle Spectrograph on the Gemini North 8.-meter telescope, he will observe the material from which planets are currently believed to be forming around young stars. The results will bear on circumstellar disk parameters such as the gas temperatures, gas dispersal time, degree of radial mixing, settling and/or growth of dust grains, and gas chemical composition at planet forming radii.These observations will follow a two-pronged approach. First Dr. Richter will search for unambiguous spectral signatures of disk emission in the pure rotational spectral lines of molecular hydrogen among 25 known circumstellar disks. The resolution of the spectrograph will allow the study of the disk line profiles from which it will be possible to infer gas temperatures and warm gas masses among the best detections. These disks will be followed up with observations of other important molecules, including water, acetylene, and hydrogen cyanide. The abundances of these molecules, along with chemical models of protoplanetary disks, will provide insight into the physical processes taking part in the planet forming regions of these young stellar systems.This project will also assure continued access by the astronomical community to this unique instrument, which fills an important gap in wavelength coverage long ward of 25 microns, offers exceptional sensitivity, and has far greater spectral resolution than is possible from space in the mid-infrared. A graduate student will also be trained in instrumentation and observing on large optical telescopes. The graduate student to be supported here will also maintain, operate and improve the spectrograph as part of a Ph.D. dissertation.

该项目将利用里希特博士部分开发的独特观测技术，以促进我们对行星起源的理解。使用得克萨斯州的梯形交叉梯形摄谱仪上的双子北8。他将使用一个100米的望远镜，观察目前被认为是在年轻恒星周围形成行星的物质。结果将影响拱星盘参数，如气体温度，气体扩散时间，径向混合程度，尘埃颗粒的沉降和/或生长，以及行星形成半径处的气体化学成分。首先，里希特博士将在25个已知的环星盘中，在氢分子的纯旋转光谱线中，寻找盘发射的明确光谱特征。光谱仪的分辨率将允许研究盘线轮廓，从中可以推断出最佳检测中的气体温度和暖气体质量。这些磁盘将与其他重要分子的观测，包括水，乙炔，和氰化氢。这些分子的丰度，沿着原行星盘的化学模型，将提供对参与这些年轻恒星系统行星形成区域的物理过程的深入了解。该项目还将确保天文学界继续使用这一独特的仪器，它填补了波长覆盖范围长达25微米的重要空白，提供了特殊的灵敏度，并且具有比中红外线的空间可能的更高的光谱分辨率。一名研究生还将接受大型光学望远镜仪器和观测方面的培训。这里支持的研究生也将维护，操作和改进光谱仪作为博士学位的一部分。论文