New radiative loss curve from updates to collisional excitation in the low-density, optically thin plasmas in SPEX

Abstract

Understanding and modelling astrophysical plasmas on atomic levels while taking into account various assumptions (for example, collisional ionisation equilibrium or photoionisation equilibrium) became essential with the progress of high-resolution X-ray spectroscopy. In order to prepare for the upcoming X-ray spectroscopy missions such as XRISM or Athena, the plasma codes with their models and the atomic databases need to be up to date and accurate. One such update for the plasma code SPEX is presented in this paper where we focus on the radiative loss due to collisional excitation in the low-density, optically thin regime. We also update the atomic data for neutral hydrogen and include the contribution of the dielectronic recombination. With all these updates being implemented in SPEX we finally present the new cooling curve. We include the comparison to other plasma codes (MEKAL, APEC, Cloudy) and other atomic databases (CHIANTI, ADAS). We show how the updated cooling impacts the stability curve for photoionised plasmas and find a new stable branch.

17 pages, 13 figures, 6 tables, accepted for publication in Astronomy & Astrophysics

References in corpus (11)

• CHIANTI - an atomic database for emission lines - Paper XV: Version 9, improvements for the X-ray satellite lines
• Atomic Data for X-ray Astrophysics
• Systematic comparison of photoionised plasma codes with application to spectroscopic studies of AGN in X-rays
• Density diagnostics of ionized outflows in active galactic nuclei: X-ray and UV absorption lines from metastable levels in Be-like to C-like ions
• X-ray spectra of the Fe-L complex
• Radiation Pressure Confinement -- III. The origin of the broad ionization distribution in AGN outflows
• Relativistic components of the Ultra-Fast Outflow in the Quasar PDS 456 from Chandra/HETGS, NuSTAR and XMM-Newton observations
• Accurate determination of the free-free Gaunt factor. II - relativistic Gaunt factors
• R-matrix electron-impact excitation data for the C-like iso-electronic sequence
• Science with hot astrophysical plasmas
• The electron energy-loss rate due to radiative recombination

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