X-Ray Evidence for Flare Density Variations and Continual Chromospheric Evaporation in Proxima Centauri

Abstract

Using the <em>XMM-Newton</em> X-ray observatory to monitor the nearest star to the Sun, Proxima Centauri, we recorded the weakest X-ray flares on a magnetically active star ever observed. Correlated X-ray and optical variability provide strong support for coronal energy and mass supply by a nearly continuous sequence of rapid explosive energy releases. Variable emission-line fluxes were observed in the He-like triplets of O VII and Ne IX during a giant flare. They give direct X-ray evidence for density variations, implying densities between 2 × 10¹⁰ and 4 × 10¹¹ cm^-3 and providing estimates of the mass and the volume of the line-emitting plasma. We discuss the data in the context of the chromospheric evaporation scenario.