Star Formation Studies in Young Star Clusters Unveiling the physical condition of young star cluster NGC 6910

Abstract

The young open cluster NGC 6910, located in the Cygnus X region, offers an excellent environment to study stellar feedback and star formation processes. Using deep UBV(RI)C photometry, Gaia EDR3 astrometry, and multiwavelength archival data (2MASS, WISE, Hα, CO), we determine the cluster’s physical parameters. NGC 6910 is found to be <10 Myr old and at a distance of ~1.7–2.0 kpc, exhibiting variable reddening. The presence of massive OB stars, pre-main-sequence members, and Class I/II YSOs indicates ongoing star formation. Spatial association among ionized gas, warm dust, and YSOs suggests feedback-triggered star formation driven by massive stars. The results highlight NGC 6910 as a dynamically active region shaping its environment through stellar feedback.