ESO的中子星天文学：VLT十年
Neutron Star Astronomy at ESO: the VLT decade
摘要：
蟹状星云脉冲星（PSR B 0531 +21）的光学识别已经过去了40年，现在已经识别出25颗不同类型的孤立中子星。欧洲南方天文台的望远镜在天文台的光学研究中发挥了关键作用，首先是拉西拉天文台的3.6米望远镜和新技术望远镜（NTT），1998年之后是帕拉纳尔天文台的甚大望远镜（VLT）。在这篇综述中，我总结了十年来孤立中子星的VLT观测中获得的一些最重要的结果。
英文摘要：
Forty years have gone by since the optical identification of the Crab pulsar (PSR B0531+21), and 25 isolated neutron stars of different types have been now identified. Observations with ESO telescopes historically played a pivotal role in the optical studies of INSs, first with the 3.6m telescope and the New Technology Telescope (NTT), at the La Silla Observatory, and after 1998 with the Very Large Telescope (VLT), at the Paranal Observatory. In this review I summarise some of the most important results obtained in ten years of VLT observations of isolated neutron stars.
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