Resonant Auger Destruction and Iron K-Alpha Spectra in Compact X-ray Sources
arXiv:astro-ph/0502002 · doi:10.1063/1.1960918
Abstract
We examine the effects of resonant Auger destruction in modifying the intensities and flux distributions of K-alpha spectra from iron L-shell ions. Applications include X-ray irradiated stellar winds in X-ray binaries and accretion disk atmospheres. Using detailed atomic models, we find that resonant Auger destruction is selective, in that only a subset of the emitted K-alpha lines is highly attenuated. We also show that that the local excitation conditions can have a dramatic effect on the K-alpha emissivity spectrum.
10 pages, PDF format only; to appear in the proceedings of X-ray Diagnostics for Astrophysical Plasmas: Theory, Experiment, and Observation, ed. R. K. Smith (Melville: AIP)
Cited by in corpus (7)
- X-ray reflected spectra from accretion disk models. III. A complete grid of ionized reflection calculations
- X-ray Absorption and Reflection in Active Galactic Nuclei
- X-ray reflected spectra from accretion disk models.II. Diagnostic tools for X-ray observations
- X-ray spectroscopy in the microcalorimeter era I: Effects of Fe XXIV Resonance Auger Destruction on Fe XXV K spectra
- A population of isolated hard X-ray sources near the supernova remnant Kes 69
- X-ray spectroscopy in the microcalorimeter era 4: Optical depth effects on the soft X-rays studied with CLOUDY
- Probing spectral and timing properties of the X-ray pulsar RX J0440.9+4431 in the giant outburst of 2022-2023