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Similarities between the X-Ray Light Curves of the 2016 and 2020 Eruptions of the Recurrent Nova LMC 1968
Research Notes of the AAS Pub Date : 2020-08-18 , DOI: 10.3847/2515-5172/abae72
Greg J. Schwarz 1 , Kim L. Page 2 , Paul M. Kuin 3 , Matthew J. Darnley 4
Affiliation  

The latest eruption of the recurrent nova LMC 1968 was extensively observed by Swift with its X-ray Telescope instrument. A comparison with the Swift data set from the 2016 eruption shows that the X-ray evolution was remarkably similar just as the evolution of the optical photometry and spectroscopy was similar during previously observed eruptions. The only difference is a surprising decrease in the recurrence time. LMC 1968 is only the second nova for which Swift has observed the entire X-ray evolution more than once. At 50 kpc, it is close enough to be extensively observed in its next eruption.

中文翻译:

经常性新星LMC 1968的2016年和2020年爆发的X射线光曲线之间的相似性

斯威夫特(Swift)的X射线望远镜仪器广泛观测到了复发性新星LMC 1968的最新喷发。与2016年喷发的Swift数据集进行的比较表明,X射线的演化非常相似,就像先前观测到的爆发期间的光学测光和光谱学的演化相似。唯一的不同是重复时间的惊人减少。LMC 1968只是斯威夫特不只一次观察到整个X射线演化的第二颗新星。在50 kpc时,它足够接近,可以在下一次喷发时被广泛观察到。
更新日期:2020-08-31
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