Evidence for Resonance Line Scattering in the Suzaku X-ray Spectrum of the Cygnus Loop
arXiv:0801.4418 · doi:10.1093/pasj/60.3.521
Abstract
We present an analysis of the Suzaku observation of the northeastern rim of the Cygnus Loop supernova remnant. The high detection efficiency together with the high spectral resolution of the Suzaku X-ray CCD camera enables us to detect highly-ionized C and N emission lines from the Cygnus Loop. Given the significant plasma structure within the Suzaku field of view, we selected the softest region based on ROSAT observations. The Suzaku spectral data are well characterized by a two-component non-equilibrium ionization model with different best-fit values for both the electron temperature and ionization timescale. Abundances of C to Fe are all depleted to typically 0.23 times solar with the exception of O. The abundance of O is relatively depleted by an additional factor of two compared with other heavy elements. We found that the resonance-line-scattering optical depth for the intense resonance lines of O is significant and, whereas the optical depth for other resonance lines is not as significant, it still needs to be taken into account for accurate abundance determination.
10 pages, 5 figures. accepted for Publications of the Astronomical Society of Japan
References in corpus (2)
Cited by in corpus (9)
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- Plasma Diagnostics of the Supernova Remnant N132D Using Deep XMM-Newton Observations with the Reflection Grating Spectrometer
- X-ray Emission from Charge Exchange in the Cygnus Loop SNR
- The Abundance Inhomogeneity in the Northern Rim of the Cygnus Loop
- Evidence for Resonance Scattering in the X-ray Grating Spectrum of the Supernova Remnant N49