Analytical study of the newly discovered open cluster Gulliver 1

E. Elhosseiny, M. N. Ismail, A. Tadross, R. El-Bendary, H. Selim, A. H. Ibrahim
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Abstract

ABSTRACT In this work, the astrophysical parameters of the open cluster Gulliver 1 are calculated using Gaia DR2 catalogue. The parameters that covered under this study are the radius, distance, colour excess, age, total mass and relaxation time also the parallax and proper motion values in both coordinates Ra and Dec beside studying the luminosity and mass functions of the cluster. Using the radial density profile, radius is found to be 6.8 ± 0.2 arcmin. We get the distance and age from the colour magnitude diagram to be 2818.38 ± 11 pc and 1.78 Gyr ±20 Myr, respectively. the horizontal-projected distances from the sun on the galactic plane X⊙ & Y⊙, the distance from the galactic plane Z⊙ and the distance from the galactic centre Rgc are obtained as 507.5 ± 2 pc, −2222 ± 8.7 pc, −1657.4 ± 6.5 pc and 3609 ± 14 pc respectively. Also, astrometric parameters are obtained such as parallax and proper motions in both coordinates Ra and Dec as 0.31 ± 0.08 mas, −7.9 ± 0.14 mas/yr and 3.6 ± 0.08 mas/yr, respectively. From the estimated relaxation time we inferred that the cluster is relaxed and has a mass of 146.2 Mʘ. Some parameters are presented for the first time.
新发现疏散星团格列佛1号的分析研究
本文利用Gaia DR2星表计算了疏散星团格列佛1的天体物理参数。除了研究星系团的光度和质量函数外,本文还研究了星系团的半径、距离、色差、年龄、总质量和弛豫时间,以及Ra和Dec坐标系下的视差和固有运动值。利用径向密度剖面,半径为6.8±0.2弧分。我们从色星等图中得到距离和年龄分别为2818.38±11 pc和1.78 Gyr±20 Myr。在银道平面X⊙、Y⊙、Z⊙和银道中心Rgc的水平投影距离分别为507.5±2 pc、- 2222±8.7 pc、- 1657.4±6.5 pc和3609±14 pc。在Ra和Dec坐标系下,视差和固有运动分别为0.31±0.08 mas、−7.9±0.14 mas/yr和3.6±0.08 mas/yr。根据估计的弛豫时间,我们推断该星团是弛豫的,质量为146.2 M。一些参数是首次提出的。
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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