| Name: Sneha Nedhath Divakaran |
| Affiliation: INAF - Osservatorio Astrofisico di Arcetri |
| Conference ID: ASI2026_653 |
| Title: AstroSat/UVIT Study of NGC 663: First detection of Be+sdOB systems in a young star cluster |
| Abstract Type: Poster |
| Abstract Category: Stars, Interstellar Medium, and Astrochemistry in Milky Way |
| Author(s) and Co-Author(s) with Affiliation: Sneha Nedhath(INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy), Sharmila Rani(INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy), Annapurni Subramaniam(Indian Institute of Astrophysics, Koramangala, Bangalore 560034, India), Elena Pancino(INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy) |
| Abstract: Be stars are rapidly rotating stars surrounded by a disc; however, the origin of these stars remains unclear. Mass and angular momentum transfer in close binaries account for the rapid rotation of a significant fraction of Be stars, as supported by the previous detection of low-mass stripped companions to these stars. The stripped companions can be helium-burning subdwarf OB-type stars (sdOBs) and white dwarfs. The main objective of this study is to characterise the identified Be stars in the young open cluster NGC 663 and search for possible hot companions. We present the first ultraviolet (UV) photometric study of NGC 663 using far-UV and near-UV data from UVIT/AstroSat. We identified 23 previously known Be stars in the cluster. Further, we utilised the spectral energy distribution fitting technique to derive the fundamental parameters and to search for UV-bright companions of the identified Be stars. Our study reveals that 19 out of 23 Be stars show a significant UV excess, indicating the presence of hot companions. Here, we report the first detection of high-mass sdOB companions to Be stars, with 69.5% of them found in binaries within a cluster, offering direct evidence of binary interactions. This study showcases the key role of binary interactions in the formation of Be stars in clusters and provides insights into massive star evolution. |
