脉冲星故障子结构和脉冲星内部
Pulsar glitch substructure and pulsar interiors
摘要：
普莱森特山天文台的脉冲星计时集中在船帆座上，可以在一天中跟踪18个小时。这些几乎连续的计时记录延续了24年，使我们能够深入了解计时噪声、微小故障和其他更奇特的影响。已经发现，船帆座脉冲星的自旋瞬间发生在数据的不确定性范围内。新的，更高分辨率的数据，揭示中子星内部的见解的潜力进行了讨论。
英文摘要：
Pulsar timing at the Mt Pleasant observatory focused on Vela, which could be tracked for 18 hours of the day. These nearly continuous timing records extend over 24 years allowing a great insight into details of timing noise, micro glitches and other more exotic effects. It has been found that the spin up for the Vela pulsar occurs instantaneously to within the uncertainties of the data. The potential for new, higher resolution data, to unveil insights of the Neutron Star interiors is discussed.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
