NY Her: possible discovery of negative superhumps

Q4 Physics and Astronomy

Information Bulletin on Variable Stars Pub Date : 2017-09-25 DOI:10.22444/IBVS.6216

A. Sosnovskij, E. Pavlenko, N. Pit, K. Antoniuk

引用次数: 1

Abstract

We presents result of CDD photometry for SU UMa dwarf nova NY Her during 6 nights in June 2017 when object was in quiescence. Light curves clearly show strong amplitude variations in a range of 0m.7-1m.1. Time series analysis revealed a period 0.07141(5) d, that we identified as the period of possible negative superhumps of NY Her.

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NY Her：负超凸点的可能发现

本文报道了2017年6月6夜对SU UMa矮新星NY Her的CDD光度测量结果。光曲线在0m.7 ~ 1m.1范围内明显表现出强烈的振幅变化。时间序列分析显示了0.07141(5)d的周期，我们认为这是NY Her可能的阴性超峰期。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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