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Ion Storage Ring Measurements of Low Temperature Dielectronic Recombination Rate Coefficients for Modeling X-Ray Photoionized Cosmic Plasmas
| Content Provider | Semantic Scholar |
|---|---|
| Author | Savin, D. W. Schwalm, D. U. Gwinner, Gerald Wolf, Andreas Mueller, Alfred Schippers, Stefan |
| Copyright Year | 2002 |
| Abstract | Low temperature dielectronic recornbinatiori (DR) is tohe clorrtirianb r.ec:orribina!,iorr rrtedianism for most ions in X-ray photoionized cosmic plasmas. Reliably modeling and interpreting spectra from these plasmas requires accuratc low tempcraturc DR ratc Coefficients. Of particular importance are the DR rate coefficients for the iron L-shell ions (Fe XvlI-Fe X X I V ) . These ions are predicted to play an important role in determining the thermal structure and line emission of X-ray photoionized plasmas, which form in the media surrounding accretion powered sources such as X-ray binaries (XRBs), active galactic nuclei (AGN), and cataclysmic variables (Savin et al., 2000). |
| File Format | PDF HTM / HTML |
| DOI | 10.7916/D8XS63RQ |
| Alternate Webpage(s) | https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/20030058910.pdf |
| Alternate Webpage(s) | https://doi.org/10.7916/D8XS63RQ |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |
