论文标题
从SN2010DA到NGC 300 ULX-1：NGC 300中不寻常的高质量X射线二进制的十年观察
From SN2010da to NGC 300 ULX-1: Ten Years of Observations of an Unusual High Mass X-ray Binary in NGC 300
论文作者
论文摘要
2010年5月，南非业余天文学家在附近的Galaxy NGC 300中发现了中间光度瞬变。自发现以来的十年中，对被错误姓名的``SN 2010da''的多波长观察不断重新塑造我们对这个高质量X射线二进制系统的理解。在这篇综述中，我们概述了多波长观测值以及试图了解2010年瞬态事件的尝试，后来将该系统重新分类为NGC〜300 ulx-1：红色超级 +中子 +中子星超级X射线源。
In 2010 May, an intermediate luminosity optical transient was discovered in the nearby galaxy NGC 300 by a South African amateur astronomer. In the decade since its discovery, multi-wavelength observations of the misnamed ``SN 2010da'' have continually re-shaped our understanding of this high mass X-ray binary system. In this review, we present an overview of the multi-wavelength observations and attempts to understand the 2010 transient event and, later, the re-classification of this system as NGC~300 ULX-1: a red supergiant + neutron star ultraluminous X-ray source.
