Toward a Complete Understanding of Young Neutron Stars

中子星是大质量恒星演化的终点，在密度和磁场的极端条件下是有价值的物质探测器。年龄小于1万年的中子星对于研究核心坍缩的物理学、核密度下物质的性质以及天体物理粒子加速器的工作非常重要。年轻的中子星性质各异，很难被发现。卡米洛博士和他的团队将通过详细分析来自无线电波长的大规模调查的现有数据，对年轻的中子星进行三次互补搜索。这些数据是对中子星最敏感的电流探测器，至少在下一代射电望远镜出现之前是如此。他的工作目标是全面了解为明亮的气体星云提供能量的年轻中子星的特性，确定新发现的一类高磁场年轻中子星的出生率，并描述瞬态射电源的性质。本研究计划也将强调研究生的训练，以及高中学生和教师参与第一线的科学探究，以增加他们对科学的理解和欣赏。现有的调查数据也将提供给更广泛的天文学界。

Neutron stars are the evolutionary end points of massive stars and are valuable probes of matter under extreme conditions of density and magnetic fields. Neutron stars with ages less than 10,000 years are extremely important for studying physics of core collapse, the properties of matter at nuclear densities, and the workings of astrophysical particle accelerators. Young neutron stars are heterogeneous in their properties, and very hard to find. Dr. Camilo and his group will undertake three complementary searches for young neutron stars by a detailed analysis of existing data from large-scale surveys at radio wavelengths. These data are the most sensitive current probes of neutron stars, at least until the advent of the next generation of radio telescopes. The goals of his work will be to obtain a full picture of the properties of young neutron stars that power bright gaseous nebulae, to determine the birthrate of a newly identified class of high magnetic field young neutron stars, and to characterize the nature of transient radio sources.This research project will also emphasize the training of graduate students and the involvement of high school students and teachers in frontline scientific inquiry, with a view toward increasing their understanding and appreciation of science. The existing survey data will also be made available to the wider astronomical community.