Photometric and Kinematic study of the open cluster NGC 1027

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Photometric and Kinematic study of the open cluster NGC 1027
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Indian astronomers investigate open cluster NGC 1027 arxiv

We present photometric and kinematic analysis of an intermediate age open cluster NGC 1027 using $UBV_c$ and Gaia Early Data Release 3 data. Structural and fundamental parameters such as cluster center, cluster extent, reddening, age and distance are estimated in this study. Cluster center is found about 2 arcmin away from the center reported earlier. Radius has been estimated to be about 8.00 arcmin.

Few stars having P$_\mu>$ 70\% are found out of the cluster radius showing imprints of dynamical evolution. The color-color and color-magnitude diagrams for the cluster members found within 8.00 arcmin have been constructed using $UBV_c$ photometry and Gaia EDR3 data. This yields a reddening E $\sim$ 0.36 mag, age $\sim$ 130 Myr and distance $\sim$ 1.14 kpc. The mass function slope in the cluster region is $\Gamma$ $\sim$ -1.46 $\pm$ 0.15, which is similar to other Galactic open clusters.

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