Discovery of X-ray flaring activity in the Arches cluster
Renzo Capelli, Robert S. Warwick, Nico Cappelluti, Stefan Gillessen,, Peter Predehl, Delphine Porquet, Stefan Czesla

TL;DR
This study reports the discovery of a significant X-ray flare in the Arches cluster, revealing insights into stellar activity and wind interactions over an 8-year observational period.
Contribution
It provides the first detailed analysis of a transient X-ray flare in the Arches cluster, linking stellar activity to observed X-ray variability.
Findings
70% increase in X-ray emission during flare
Flare duration longer than four days
No change in temperature or column density during flare
Abstract
We present a study of the Arches cluster based on XMM-Newton observations performed over the past 8 years. Unexpectedly, we find that the X-ray emission associated with the cluster experienced a marked brightening in March/April 2007. We investigate the origin of both the X-ray continuum emission emanating from the star cluster and the flare. To study the time variability of the total X-ray flux, we stacked the PN and MOS data of observations performed within a time interval of a few days leading to the detection of the flaring episode. We then constructed two spectral datasets, one corresponding to the flare interval (March/April 2007) and another to the normal quiescent state of the source. The X-ray light curve of the Arches cluster shows, with high significance (8.6 sigma), a 70% increase in the X-ray emission in the March/April 2007 timeframe followed by a decline over the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
