[Fe XIV] and [Fe XI] reveal the forward shock in SNR 1E 0102.2-7219

@article{Vogt2017FeXA,
  title={[Fe XIV] and [Fe XI] reveal the forward shock in SNR 1E 0102.2-7219},
  author={Fr{\'e}d{\'e}ric P. A. Vogt and Ivo R. Seitenzahl and Michael A. Dopita and P.Ghavamian},
  journal={Astronomy and Astrophysics},
  year={2017},
  volume={602}
}
Aims. We study the forward shock in the oxygen-rich young supernova remnant (SNR) 1E0102.2-7219 (1E0102 in short) via optical coronal emission from [Fe XIV] and [Fe XI]: emission lines which offer an alternative method to X-rays to do so. Methods. We have used the Multi-Unit Spectroscopic Explorer (MUSE) optical integral field spectrograph at the Very Large Telescope (VLT) on Cerro Paranal to obtain deep observations of SNR 1E0102 in the Small Magellanic Cloud. Our observations cover the… 

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