John C. Raymond

TL;DR: The Astrophysical Plasma Emission Code (APEC) as mentioned in this paper uses atomic data from the companion ASTPED database to calculate spectral models for hot plasmas, such as collisional and radiative rates, recombination cross sections, dielectronic recombination rates, and satellite line wavelengths.

TL;DR: In this article, the authors report direct observations of the magnetic reconnection site during an eruptive process that occurred on 2003 November 18, which started with a rapid expansion of a few magnetic arcades located over the east limb of the Sun and developed an energetic partial-halo coronal mass ejection (CME), a long current sheet and a group of bright flare loops in the wake of the CME.

TL;DR: In this article, the authors present an observational and theoretical study of the optical emission from nonradiative shocks in three supernova remnants: the Cygnus Loop, RCW 86, and Tycho.

TL;DR: In this article, the authors present mocassin two-dimensional photoionization and dust radiative transfer models of a prototypical T Tauri disk irradiated by X-rays from the young pre-main-sequence star.

TL;DR: In this article, the authors report on simultaneous ChandraHETGS andRXTE observations of the transient stellar-mass black hole GRO J1655�40, made during its 2005 outburst, revealing a line-rich X-ray absorption spectrum consistent with a diskwind.