首页> 外文期刊>Astronomy and astrophysics >Mean angular diameters, distances, and pulsation modes of the classical Cepheids FF?Aquilae and T?Vulpeculae - CHARA/FLUOR near-infrared interferometric observations
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Mean angular diameters, distances, and pulsation modes of the classical Cepheids FF?Aquilae and T?Vulpeculae - CHARA/FLUOR near-infrared interferometric observations

机译:经典造父变星FF?Aquilae和T?Vulpeculae的平均角直径,距离和脉动模式-CHARA / FLUOR近红外干涉测量观察

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We report the first angular diameter measurements of two classical Cepheids, FF?Aql and T?Vul, that we obtain using observations with the FLUOR instrument installed at the CHARA interferometric array. We derive average limb-darkened angular diameters of θLD?=?0.878?±?0.013?mas and θLD?=?0.629?±?0.013?mas, respectively, for FF?Aql and T?Vul. Combining these angular diameters with the HST-FGS trigonometric parallaxes leads to linear radii R?=?33.6?±?2.2???R⊙ and R?=?35.6?±?4.4???R⊙, respectively. The comparison with empirical and theoretical period–radius relations leads to the conclusion that these Cepheids are pulsating in their fundamental mode. The knowledge of this pulsation mode is of prime importance to calibrating the period–luminosity relation with a uniform sample of fundamental mode Cepheids.
机译:我们报告了两个经典造父变星FF?Aql和T?Vul的首次角直径测量结果,这是通过使用安装在CHARA干涉仪阵列上的FLUOR仪器的观测结果获得的。对于FFΔAql和TΔVul,我们分别得出平均肢体变暗的角直径为LDLD =0.878Ω±0.013mas和θLD≥0.629Ω±0.013mas。将这些角直径与HST-FGS三角视差相结合,分别得出线性半径R 1 = 33.6±±2.2 2.2 R 1和R 3 = 35.6±±4.4 4.4 R 4。与经验和理论周期-半径关系的比较得出结论:这些造父变星以其基本模式脉动。对这种脉动模式的了解对于用基本模式造父变星的统一样本校准周期-发光度关系至关重要。

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