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使用CCD VRI,盖亚DR3和2MASS对研究较少的开放星团King 18进行了深入的调查
Nasser M Ahmed1, R Bendary2, R M Samir2
1National Research Institute of Astronomy and Geophysics (NRIAG), Helwan, Cairo, 11421, Egypt. nasser_ahnmed@yahoo.com.
Scientific reports
|October 10, 2024
概括
这项研究使用Gaia DR3和其他观测数据重新估计了年轻的开放星团King 18的天体物理参数. 发现King 18是一个动态稳定和放松的星团,估计年龄为2.24亿年.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 恒星进化 恒星进化
背景情况:
- 王18是一个研究较少的年轻开放星团.
- 准确的天体物理参数对于理解星团动态和演变至关重要.
研究的目的:
- 重新估计18号国王的天文和光学参数.
- 通过使用新数据来确定会员和天体物理参数.
- 评估18号国王的动态状态和稳定性.
主要方法:
- 使用了盖亚数据发布3 (DR3),两微米全天文调查 (2MASS) 和VRI CCD观测.
- 使用来自科塔米亚天文台 (KAO) 的数据.
- 计算了集群中心,半径,密度分布,颜色大小图,距离,年龄和红色.
主要成果:
- 估计质量函数斜率为2.27±0.17,与萨尔佩特值相比.
- 确定了平均集群年龄为224 ± 6.3 Myrs,放松时间为28.92 Myrs.
- 计算的距离从2857.59到2992.26pc之间,颜色过度为E(V-I),E(J-K和E(B-V).
结论:
- 证实18号王星团是一个动态稳定和放松的开放星团.
- 该研究为18号国王提供了最新和可靠的天体物理参数.
- 这些发现有助于更好地了解年轻的开放星团.
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