High-resolution spectroscopy of NGC 300 OT2008-1 identifies more emission lines and complex ejecta profiles than low-resolution data, showing that HR monitoring is needed to avoid misleading inferences about transient energetics and geometry.
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The benefit of a multi-band high resolution spectroscopic monitoring for studying stellar transients: the NGC 300 OT2008-1 UVES spectrum as a test case
High-resolution spectroscopy of NGC 300 OT2008-1 identifies more emission lines and complex ejecta profiles than low-resolution data, showing that HR monitoring is needed to avoid misleading inferences about transient energetics and geometry.