Searching for Variable Stars in the Open Cluster NGC 2355 and Its Surrounding Region

• Published in: The Astronomical journal 2022-08, Vol.164 (2), p.40
• Main Authors: Wang, Hong, Zhang, Yu, Zeng, Xiangyun, Hu, Qingshun, Liu, Jinzhong, Qin, Mingfeng, Lü, Guoliang
• Format: Article
• Language: English
• Subjects: Astronomy; Astronomy data analysis; Binary stars; Clusters; Color; Eclipsing binary stars; Homogeneity; Kinematics; Light curve; Lunar eclipses; Open star clusters; Parallax; Photometric observations; Photometry; Physical properties; Stellar rotation; Variable stars
• ISSN: 0004-6256; 1538-3881
• DOI: 10.3847/1538-3881/ac755a

We have investigated the variable stars in the field surrounding NGC 2355 based on the time-series photometric observation data. More than 3000 CCD frames were obtained in the V band spread over 13 nights with the Nanshan One-meter Wide-field Telescope. We have detected 88 variable stars, containing 72 new variable stars and 16 known variable stars. By analyzing these light curves, we classified the variable stars as follows: 26 eclipsing binaries, 52 pulsating stars, four rotating variables, and six unclear type-variable stars for which their periods are much longer than the time baseline chosen. Employing Gaia DR2 parallax, kinematics, and photometry, the cluster memberships of these variable stars were also analyzed for NGC 2355. In addition to the 11 variable members reported by Cantat-Gaudin et al. (2018), we identify four more variable member candidates located at the outer region of NGC 2355 and showed homogeneity in space positions and kinematic properties with the cluster members. The main physical parameters of NGC 2355 estimated from the two-color and color–magnitude diagrams are log(age/yr) = 8.9, E ( B − V ) = 0.24 mag, and [Fe/H] = −0.07 dex.