The bulge globular cluster Terzan 6 as seen from multi-conjugate adaptive optics and HST★

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2025-03-18 DOI:10.1051/0004-6361/202453482
M. Loriga, C. Pallanca, F. R. Ferraro, E. Dalessandro, B. Lanzoni, M. Cadelano, L. Origlia, C. Fanelli, D. Geisler, S. Villanova
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Abstract

This work consists of the first detailed photometric study of Terzan 6, one of the least known globular clusters in the Galactic bulge. Through the analysis of high angular resolution and multiwavelength data obtained from adaptive optics corrected and space observations, we built deep, optical and near-infrared color-magnitude diagrams reaching ≈4 magnitudes below the main-sequence turnoff. Taking advantage of four different epochs of observations, we measured precise relative proper motions for a large sample of stars, from which cluster members have been solidly distinguished from Galactic field interlopers. A noncanonical reddening law (with RV = 2.85) and high-resolution differential reddening map, with color excess variations up to δE(BV) ≈ 0.8 mag, have been derived in the direction of the system. According to these findings, new values for the extinction and distance modulus have been obtained: E(BV) = 2.36 ± 0.05 and (mM)0 = 14.46 ± 0.10 (corresponding to d = 7.8 ± 0.3 kpc), respectively. We also provide the first determinations of the cluster center and projected density profile from resolved star counts. The center is offset by more than 7″ to the east from the literature value, and the structural parameters obtained from the King model fitting to the density profile indicate that Terzan 6 is in an advanced stage of its dynamical evolution, with a large value for the concentration parameter (c = 1.94−0.26+0.24) and a small core radius (rc = 2.6−0.7+0.09 arcsec). We also determined the absolute age of the system, finding t = 13 ± 1 Gyr, in agreement with the old ages found for the globular clusters in the Galactic bulge. From the redetermination of the absolute magnitude of the red giant branch bump and the recent estimate of the cluster global metallicity, we find that Terzan 6 nicely matches the tight relation between these two parameters drawn by the Galactic globular cluster population.
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用多共轭自适应光学和HST观察的球状星团泰山6
这项工作包括对泰山6号的第一次详细的光度研究,泰山6号是银河系凸起中最不为人知的球状星团之一。通过对自适应光学校正和空间观测获得的高角分辨率和多波长数据的分析,我们建立了在主序关断下≈4等的深、光学和近红外色星等图。利用四个不同时期的观测,我们测量了大量恒星样本的精确相对固有运动,从这些样本中,星团成员已经与银河系场的闯入者明确区分开来。在系统方向上推导出了非正则变红规律(RV = 2.85)和高分辨率差分变红图,其颜色过量变化高达δE(B−V)≈0.8等。根据这些发现,得到了消光模量和距离模量的新值:E(B−V) = 2.36±0.05和(m−m)0 = 14.46±0.10(对应d = 7.8±0.3 kpc)。我们还提供了星团中心的第一个确定,并通过分辨恒星计数预测了密度剖面。中心较文献值偏东7″以上,King模型拟合密度剖面得到的结构参数表明,特赞6号处于动力学演化的晚期,浓度参数值较大(c = 1.94 ~ 0.26+0.24),核芯半径较小(rc = 2.6 ~ 0.7+0.09 arcsec)。我们还确定了这个系统的绝对年龄,发现t = 13±1 Gyr,与银河系凸起的球状星团的年龄一致。通过重新确定红巨星分支凸起的绝对星等和最近对星团全球金属丰度的估计,我们发现Terzan 6很好地匹配了银河系球状星团人口绘制的这两个参数之间的紧密关系。
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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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