Journal ArticleDOI
Soft X-ray spectrum of a hot plasma.
John C. Raymond,Barham W. Smith +1 more
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TLDR
The spectrum of radiation emitted by a hot optically thin plasma with abundances and equilibrium ionization balance appropriate to interstellar conditions has been calculated in this article for wavelengths shorter than 200 A.Abstract:
The spectrum of radiation emitted by a hot optically thin plasma with abundances and equilibrium ionization balance appropriate to interstellar conditions has been calculated. The results at wavelengths shorter than 200 A are discussed for material in the electron-temperature range from 160,000 to 100 million K.read more
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Collisional Plasma Models with APEC/APED: Emission-Line Diagnostics of Hydrogen-like and Helium-like Ions
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.
Journal ArticleDOI
Statistical Properties of X-Ray Clusters: Analytic and Numerical Comparisons
TL;DR: The authors compare the results of Eulerian hydrodynamic simulations of cluster formation against virial scaling relations between four bulk quantities: the cluster mass, the dark matter velocity dispersion, the gas temperature, and the cluster luminosity.
Journal ArticleDOI
Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
TL;DR: The authors compare the results of Eulerian hydrodynamic simulations of cluster formation against virial scaling relations between four bulk quantities: the cluster mass, the dark matter velocity dispersion, the gas temperature and the cluster luminosity.
Journal ArticleDOI
The Treatment of Non-LTE Line Blanketing in Spherically Expanding Outflows
TL;DR: In this article, the authors proposed to use the idea of super levels first pioneered by Anderson to improve the performance of the non-LTE radiative transfer code of Hillier stars with stellar winds.
Journal ArticleDOI
Starburst-driven Mass Loss from Dwarf Galaxies: Efficiency and Metal Ejection
TL;DR: In this paper, the effects of repeated supernova (SN) explosions from starbursts in dwarf galaxies on the interstellar medium of these galaxies, taking into account the gravitational potential of their dominant dark matter halos, were explored.
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