论文标题

搜索苔丝全帧图像中的可变细分b星 - I.南方黄半球的可变物体

A search for variable subdwarf B stars in TESS Full Frame Images -- I. Variable objects in the southern ecliptic hemisphere

论文作者

Sahoo, S. K., Baran, A. S., Sanjayan, S., Ostrowski, J.

论文摘要

我们报告了我们在全画幅图像中搜索脉动细分B星的搜索结果,并在30分钟的节奏中采样,并在苔丝任务的第1年内收集。 1年级覆盖了大部分南方的黄半球。我们检查的对象样本是从可公开可用于公共的SubdWarf B星星数据库中选择的。但是,作为我们搜索的副产品,我们发现了1807个变量对象,其中大多数未分类,因此无法确认它们的特定可变性类别。我们的初步发现包括:两个新的B(SDB)脉动器,26个带有已知SDB光谱的变量,83个非分类脉动恒星,83个黯然失色的二进制文件(分离和半透射),1535个脉动脉动脉动脉动脉动的混合物和非分类的bineae,两个Noviae,两个Noviarbles,and 77 variables and 77 variables,and 77 variables和77 variables和77 variables and 77 variables and 77 variables,以及77个变量。在黯然失色的二进制文件中,我们确定了两个已知的HW VIR系统和四个新候选者。两个SDB脉动器的振幅光谱不丰富,但我们得出了其中一个模态度的估计值。此外,我们在83个脉动器中选择了五个SDBV候选者进行模式识别,并根据此初步分析描述了我们的结果。进一步的进展将需要新发现的变量星的光谱分类,希望其中包括更多的B恒星。

We report the results of our search for pulsating subdwarf B stars in Full Frame Images, sampled at 30 min cadence and collected during Year 1 of the TESS mission. Year 1 covers most of the southern ecliptic hemisphere. The sample of objects we checked for pulsations was selected from a subdwarf B stars database available to public. Only two positive detections have been achieved, however, as a by-product of our search we found 1807 variable objects, most of them not classified, hence their specific variability class cannot be confirmed at this stage. Our preliminary discoveries include: two new subdwarf B (sdB) pulsators, 26 variables with known sdB spectra, 83 non-classified pulsating stars, 83 eclipsing binaries (detached and semi-detached), a mix of 1535 pulsators and non-eclipsing binaries, two novae, and 77 variables with known (non-sdB) spectral classification. Among eclipsing binaries we identified two known HW Vir systems and four new candidates. The amplitude spectra of the two sdB pulsators are not rich in modes, but we derive estimates of the modal degree for one of them. In addition, we selected five sdBV candidates for mode identification among 83 pulsators and describe our results based on this preliminary analysis. Further progress will require spectral classification of the newly discovered variable stars, which hopefully include more subdwarf B stars.

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