The persistent Be enigma: The case of HD 212044

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2024-10-29 DOI:10.1051/0004-6361/202452215
Alan W. Pereira, Eduardo Janot-Pacheco, Laerte Andrade, Marcelo Emilio
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Abstract

We present an analysis of the Be star HD 212044 that reveals intriguing correlations between photometric variations, circumstellar disk emission, and frequencies. Our findings, based on data from the Transiting Exoplanet Survey Satellite (TESS) mission, show an unexpectedly strong negative correlation between photometric brightness and Hα equivalent width, challenging the established understanding of the behavior of Be star seen at low inclination angles. Notably, beating episodes precede brightening events. This study suggests that the variability of HD 212044 may be due to additional mechanisms.
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持续存在的Be之谜:HD 212044的情况
我们对Be恒星HD 212044进行了分析,揭示了测光变化、周星盘发射和频率之间有趣的相关性。我们的研究结果基于凌日系外行星巡天卫星(TESS)任务的数据,显示出测光亮度与Hα等效宽度之间出乎意料的强烈负相关,挑战了人们对低倾角Be星行为的既定理解。值得注意的是,跳动事件发生在变亮事件之前。这项研究表明,HD 212044 的变化可能是由其他机制造成的。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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