老新星:昔日辉煌,未来光明

黄金时代 Pub Date : 2018-06-06 DOI:10.22323/1.315.0045
A. Ederoclite, C. Tappert, L. Schmidtobreick, N. Vogt
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引用次数: 0

摘要

经典新星是重要的天体物理实验室,在现代天文学的几个方面具有极其重要的意义。要全面了解新星现象,不仅要了解新星明亮的阶段,还要了解这些事件发生的双星的特性。本文主要讨论了30多年前发生新星爆炸的巨变星(cv)的性质。对这些对象进行了CV总体和其最大属性的分析。最后,我们建议读者在正确的步骤,以便在盖亚时代使用旧新星。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Old Novae: Old Glories with Bright Future
Classical novae are important astrophysical laboratories and are extremely relevant in several aspects of modern astronomy. A complete understanding of the nova phenomenon passes through the understanding not only of the phase where the nova is bright, but also understanding the properties of the binaries in which these events occur. This paper focusses on the properties of Cataclysmic Variables (CVs) which have harboured a nova explosion more than 30 years ago. The objects are analysed both in terms of CV population and in relation to their properties at maximum. Finally, we advice the reader on the proper steps in order to use old novae in the Gaia era.
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