Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …

X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally
attributed to the presence of a magnetic corona that contains plasma at temperatures …

We have analyzed a number of intense X-ray flares observed in the Chandra Orion
Ultradeep Project (COUP), a 13 day observation of the Orion Nebula Cluster (ONC) …

Determination of the length of coronal loops from the decay of X-ray flares I. S ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …

We present an X-ray observation of the eclipsing binary Algol, obtained with the BeppoSAX
observatory. During the observation a huge flare was observed, exceptional both in duration …

Abstract Pre-main-sequence (PMS) stars are known to produce powerful X-ray flares, which
resemble magnetic reconnection solar flares scaled by factors up to 10 4. However, there …

Coronal astronomy is by now a fairly mature discipline, with a quarter century having gone
by since the detection of the first stellar X-ray coronal source (Capella), and having …

Context. The diagnostics of stellar flaring coronal loops have been so far largely based on
the analysis of the decay phase. Aims. We derive new diagnostics from the analysis of the …

Past hydrodynamic simulations have been able to reproduce the high temperatures and
densities characteristic of solar flares. These simulations, however, have not been able to …

Twin X-ray flares and the active corona of AB Dor observed with BeppoSAX ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect …