“日食双星V951英仙座的第一次光度和动力学研究”的勘误表[新天文学,第119卷,2025年10月,102418]

IF 2.1 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Bin Zhang , Wei Tao , Zhen Zhong
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引用次数: 0

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本文章由计算机程序翻译,如有差异,请以英文原文为准。
Corrigendum to “The first photometric and dynamical study of the eclipsing binary star V951 Perseus” [New Astronomy, Vol 119, October 2025, 102418]
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来源期刊
New Astronomy
New Astronomy 地学天文-天文与天体物理
CiteScore
4.00
自引率
10.00%
发文量
109
审稿时长
13.6 weeks
期刊介绍: New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation. New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.
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