The Secret lives of open clusters: a multiwavelength examination of three open clusters

Star clusters are well known for their dynamical interactions, an outcome of their high stellar densities; in this paper, we use multiwavelength observations to search for the unique outcomes of these interactions in three nearby Galactic open clusters (OCs): IC 2602 (30 Myr), NGC 2632 (750 Myr), and M67 (4 Gyr). We compared X-ray observations from all-sky surveys like eROSITA, plus archival observations from Chandra X-ray Observatory, survey radio observations from ASKAP’s Evolutionary Map of the Universe survey plus archival VLA observations, in conjunction with new cluster catalogues with Gaia. From X-ray, we found 77 X-ray sources likely associated with IC 2602, 31 X-ray sources in NGC 2632, and 31 near M67’s central regions. We were further able to classify these X-ray sources based on their optical variability and any radio emission. Three IC 2602 X-ray sources had radio counterparts, which are likely all chromospherically active binary stars. We also identified luminous radio and X-ray variability from a spectroscopic triple system in M67, WOCS 3012/S1077, which is either consistent with a quiescent black hole binary, or due to an active binary stellar system. A recent population study of optical variables by Anderson & Hunt (2025) shows that the population of optical variables in OCs clearly changes over cluster age; this pilot study gives evidence that the X-ray population also changes with time and demonstrates the need for a broader multiwavelength study of Galactic OCs.