The Hidden Lives of Massive Protostars: Fragmentation, Disks, and Feedback

巨大原恒星的隐藏生活：碎片、磁盘和反馈

• 批准号: 0807739
• 负责人: Mark Krumholz
• 金额: $ 37.62万
• 依托单位: University of California-Santa Cruz
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2008
• 资助国家: 美国
• 起止时间: 2008-07-01 至 2012-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0807739&HistoricalAwards=false
• 关键词: Hidden; Lives; Massive; Protostars; Fragmentation

While there has been considerable progress toward the development of a standard model for the process of star formation in the case of low mass stars, we are much further from understanding how massive stars form. Massive stars produce most of the metals in the universe, dominate the energy balance of both the interstellar and intergalactic media via their ionizing radiation, winds, and supernovae, and shape the formation of planets through their interactions with nearby protoplanetary disks. No understanding of these processes is possible without a reliable model of massive star formation. In this project, Dr. Mark Krumholz (University of California - Santa Cruz) will develop such a model, using the complementary tools of analytic investigation and high resolution simulation including gravity, radiation, and magnetohydrodynamics.As part of this research a number of questions and problems must be addressed. At the earliest stages of massive star formation, we must understand the fragmentation process. What physical mechanisms control whether gas fragments down to sizes less than one solar mass or collapses monolithically to a massive star? Once collapse begins, any model must describe how to overcome the two dominant barriers to accretion, angular momentum and radiation pressure. Disks are a likely solution, since they redistribute angular momentum while at the same time their high opacity shields gas from radiation. A second important part of this project is to develop an understanding of massive protostellar disks. At the end of the massive star formation process, what eventually halts accretion and clears away any remaining gas? In addition to working on these questions, and using material related to this research, Dr. Krumholtz will also offer math and science courses to prison inmates in prisons near Santa Cruz, California, building on Dr. Krumholz's decade of experience in prison education. Dr. Krumholtz will involve faculty, staff, and students at UC Santa Cruz in this activity, thereby facilitating interactions between the scientific community and a radically under-served, largely minority population.

虽然在低质量恒星的情况下，星星形成过程的标准模型的发展已经取得了相当大的进展，但我们离理解大质量恒星是如何形成的还有很长的路要走。大质量恒星产生宇宙中的大多数金属，通过其电离辐射，风和超新星控制星际和星系间介质的能量平衡，并通过与附近原行星盘的相互作用塑造行星的形成。如果没有大质量星星形成的可靠模型，就不可能理解这些过程。在这个项目中，Mark Krumholz博士（加州大学-圣克鲁斯分校）将开发这样一个模型，使用分析调查和高分辨率模拟的补充工具，包括重力，辐射和磁流体力学。作为这项研究的一部分，一些问题和问题必须得到解决。在大质量星星形成的最早阶段，我们必须了解碎裂过程。是什么物理机制控制着气体碎片的大小小于一个太阳质量，还是整体坍缩成一颗大质量的星星？ 一旦坍缩开始，任何模型都必须描述如何克服吸积的两个主要障碍，即角动量和辐射压力。 光子晶体是一个可能的解决方案，因为它们重新分配角动量，同时它们的高不透明度保护气体免受辐射。该项目的第二个重要部分是发展对大质量原恒星盘的理解。 在大质量星星形成过程的最后，是什么最终阻止了吸积并清除了任何残留的气体？ 除了研究这些问题，并使用与本研究相关的材料，Krumholtz博士还将在加州的圣克鲁斯附近的监狱为监狱囚犯提供数学和科学课程，建立在Krumholz博士十年的监狱教育经验基础上。 Krumholtz博士将让加州大学圣克鲁斯分校的教职员工和学生参与这项活动，从而促进科学界与服务严重不足的少数民族之间的互动。