In CGCG 007-025, high-resolution spectroscopy resolves a kinematically distinct, asymmetric HeII line and line ratios that imply fast radiative shocks at 250-300 km/s, and shows the claimed [FeX] coronal detection is a SiII line.
Z., et al., 2022a, @doi [ ] 10.3847/1538-4357/ac7854, https://ui.adsabs.harvard.edu/abs/2022ApJ...935...74A 935
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Shocks and complex chemodynamics in the metal-poor starburst galaxy CGCG 007-025 revealed through high-resolution echelle spectroscopy
In CGCG 007-025, high-resolution spectroscopy resolves a kinematically distinct, asymmetric HeII line and line ratios that imply fast radiative shocks at 250-300 km/s, and shows the claimed [FeX] coronal detection is a SiII line.