RX 幼体的古新星外壳显示了质量转移率的演变

Krystian Iłkiewicz, Joanna Mikołajewska, Michael M. Shara, Jacqueline K. Faherty and Simone Scaringi
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引用次数: 0

摘要

RX Pup是一个共生双星,在20世纪70年代经历了一次新星爆发。在这里,我们报告在该系统周围发现了一个距今1300年的新星外壳,并可能探测到一个距今7000年的新星外壳。这使得RX Pup成为第一个观测到三个新星外壳的系统。这三次喷发表明新星的重现时间发生了变化。最有可能的解释是该系统中质量供体的进化变化导致了质量转移率的改变。值得注意的是,与理论模型的比较分析表明,在过去的一万年中,平均质量转移率增加了 3 倍。这使得 RX Pup 成为一个独特的系统,使我们能够探究双星系统中质量转移率的千年尺度演变。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Ancient Nova Shells of RX Pup Indicate Evolution of Mass Transfer Rate
RX Pup is a symbiotic binary that experienced a nova outburst in the 1970s. Here we report a discovery of a ∼1300 yr old nova shell around the system and a possible detection of a ∼7000 yr old nova shell. Together with the nova shell ejected in the 1970s, this makes RX Pup the first system with three nova shells observed. This triad of eruptions suggests a change in the nova recurrence time. The most likely explanation is an alteration in the mass transfer rate attributed to evolutionary changes of the mass donor in the system. Notably, comparative analyses with theoretical models indicate an increase in the average mass transfer rate by a factor of 3 over the past 10,000 yr. This makes RX Pup a unique system, which allows us to probe millennium-scale evolution of mass transfer rates in binary systems.
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