标题： 帕克斯射电望远镜观测到的脉冲星 显示英文标题

标题： Pulsar observations at Mt. Pleasant

摘要： 两个脉冲星每日监测计划正在澳大利亚塔斯马尼亚州霍巴特市的莫特普莱森天文台推进。 一个涉及26米射电望远镜的新系统每天监测10颗年轻脉冲星，并专注于近实时的脉冲星“跃变”探测。这将允许“机会目标”观测来测量中子星表面在“跃变”后的加热情况（Helfand, Gotthelf, & Halpern 2000）。 14米望远镜继续进行其第21个年头的维拉脉冲星每日监测，并且最近完成了前端设备的全面升级。这是在目前正在进行的后端设备升级之前完成的。 14米望远镜在2000年1月观察到了维拉脉冲星的最近一次“跃变”，达到了任何“跃变”中最高的时间分辨率，并揭示了一个特别短时的衰减成分（Dodson, McCulloch, & Lewis 2002）。 这个衰减成分将有助于限制恒星地壳与液态内部之间的耦合性质。 显示英文摘要

摘要： Two daily pulsar monitoring programs are progressing at the Mount Pleasant Observatory, Hobart, Tasmania, Australia. A new system involving the 26-metre radio telescope monitors 10 young pulsars daily and is focussed on near-real-time glitch finding. This will allow Target of Opportunity observations to measure post-glitch heating of the neutron star surface (Helfand, Gotthelf, & Halpern 2000). The 14-metre continues its 21st year of daily monitoring of the Vela pulsar with a recent comprehensive frontend upgrade. This is prior to an upgrade of the backend equipment currently in progress. The 14-metre observed the most recent glitch of the Vela pulsar in January 2000 to the highest time resolution of any glitch and revealed a particularly short-term decay component (Dodson, McCulloch, & Lewis 2002). This decay component will provide constraints to the nature of the coupling of the stellar crust to the liquid interior.