北半球最近可见新星的观测

P. Dubovský, I. Kudzej, Tomáš Medulka, Petrik Karol, S. Shugarov
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引用次数: 0

摘要

我们正在经历最近两年从北半球观测到的新星爆炸率的增加。从2020年7月强烈变红的新星V1391 Cas开始,我们连续观测到一些新星的爆发。本文报道了5颗经典新星的观测结果:Nova Cas 2020 = V1391 Cas, Nova Per 2020 = V1112 Per, Nova Cas 2021 = V1405 Cas, Nova Her 2021 = V1674 Her和Nova Vul 2021 = V606 Vul。最好的在最后-复发共生新星RS蛇夫。在本文中,我们报告了我们的光度和光谱观测结果。在不久的将来要进行彻底的分析。此时此刻,我们想强调两个重要的事实。在V1405 Cas的例子中,我们知道其前身的轨道周期。V1674 Her的前身是一个具有已知白矮星自旋周期的中间极。在这两种情况下,比较新星爆炸后的数值将是非常有趣的。在V1674 Her的例子中,我们已经测量了轨道和自旋周期。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Observations of Recent Novae Visible on the Northern Hemisphere
We are experiencing an increased rate of nova explosion observed from the northern hemisphere in the recent 2 years. Starting from July 2020 with the strongly reddened nova V1391 Cas, we are continuously observing some novae in outburst. Here, we report the observations of 5 classical novae: Nova Cas 2020 = V1391 Cas, Nova Per 2020 = V1112 Per, Nova Cas 2021 = V1405 Cas, Nova Her 2021 = V1674 Her and Nova Vul 2021 = V606 Vul. The best at the end - the recurrent symbiotic nova RS Oph. In this paper, we report our photometric and spectroscopic observations. Thorough analysis is to be done in the near future. At this moment we want to highlight two important facts. In the case of V1405 Cas, we know the orbital period of the progenitor. The progenitor of V1674 Her is an intermediate polar with known white dwarf spin period. In both cases, it will be very interesting to compare the values after the nova explosion. In the case of V1674 Her, we have already measured both the orbital and the spin period.
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