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.
@doi [ ] 10.1093/mnras/stab3150, https://ui.adsabs.harvard.edu/abs/2022MNRAS.511.2515F 511
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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.