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Optical and Infrared Photometric Study of Old Open Star Cluster Berkeley 39

机译:老开放星团伯克利的光学和红外光度研究39

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In this paper we present astrophysical parameters of the very old open star cluster Berkeley 39 using 2MASS JHK data and observation of BV CCD photometry (V ~ 21.5 mag) in Johnson-Cousin filters. We have derived reddening, distance, metallicity and age etc. using two color diagrams in near-infrared and optical bands. We have found EB-V = 0.099 ± 0.02, EJ-H = 0.018 ± 0.001 and EJ-Ks = 0.016 ± 0.001 mag, and the distance modulus of (m-M) 0 = 13.24 ± 0.03 mag, which give a distance of 4.2 ± 0.04 Kpc, and the age of the cluster is 5.6 Gyr with metallicity; Z = 0.008 (obtained from fitting of the observed CMDs with Padova iso-chrones). The radius of the cluster obtained from the analysis of 2MASS data is equal 9.0 ± 0.13 arc minutes; it reflects that the cluster have large radius with new cluster center. Luminosity and mass functions have been investigated as well as the dynamical relaxation time of the cluster Berkeley 39.
机译:在本文中,我们使用2MASS JHK数据和在Johnson-Cousin滤镜中观察BV CCD光度(V〜21.5 mag),介绍了非常老的开放星团Berkeley 39的天体参数。我们使用近红外和光学波段中的两个颜色图得出了变红,距离,金属性和寿命等。我们发现EB-V = 0.099±0.02,EJ-H = 0.018±0.001和EJ-Ks = 0.016±0.001 mag,距离模(mM)0 = 13.24±0.03 mag,得出的距离为4.2± 0.04 Kpc,簇的年龄为5.6 Gyr,具有金属性; Z = 0.008(通过将观察到的CMD与Padova等时线拟合得到)。通过分析2MASS数据获得的簇的半径等于9.0±0.13弧分;它反映出群集具有新的群集中心的较大半径。已经研究了光度和质量函数以及伯克利星团39的动力学弛豫时间。

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