We describe the 2023 release of the spectral synthesis code Cloudy. Since the previous
major release, migrations of our online services motivated us to adopt git as our version …

Solar wind charge-exchange (SWCX) emission is present in every X-ray observation of an
astrophysical object. The emission is problematic when one cannot remove the foreground …

Context. SRG/eROSITA is situated in a halo orbit around L2 where the highly variable solar
wind charge exchange (SWCX) emission from Earth's magnetosheath is expected to be …

Aims. The Gemini-Monoceros X-ray enhancement is a rich field for studying diffuse X-ray
emission and supernova remnants (SNRs). Most SNRs in this part of the sky are notoriously …

The AtomDB project provides models of X-ray and extreme ultraviolet emitting astrophysical
spectra for optically thin, hot plasma. We present the new software package, PyAtomDB …

Recent X-ray studies of starburst galaxies have found that charge exchange (CX) commonly
occurs between outflowing hot plasma and cold gas, possibly from swept-up clouds …

We report the discovery of a geocoronal solar wind charge exchange (SWCX) event
corresponding to the well‐known 2006 December 13th coronal mass ejection (CME) event …

X-ray spectra of galaxy clusters are dominated by the thermal emission from the hot
intracluster medium. In some cases, besides the thermal component, spectral models …

Charge exchange has been recognized as a primary source of soft X-ray emission in many
astrophysical outflow environments, including cometary and planetary exospheres impacted …

Single-and double-electron capture (SEC and DEC) processes occurring in O 6+ and H 2
collisions are investigated in a wide-energy domain ranging from 0.1 to 100 keV u− 1. Total …