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- W4377291234 abstract "Abstract Coronal emission lines, especially the [Fe x ] λ 6374 line, are now being used as tracers for intermediate mass black holes (IMBHs) in low-mass galaxies. We show that the recent discovery of [Fe x ] λ 6374 emission in the metal-poor starburst SDSS J094401.87-003832.1 by Reefe et al. is, in fact, a misidentified line. The line interpreted as [Fe x ] λ 6374 is Si ii λ 6371. We caution that current and future campaigns hunting for IMBHs with the [Fe x ] λ 6374 line need to account for possible contamination by Si ii λ 6371 emission." @default.
- W4377291234 created "2023-05-23" @default.
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- W4377291234 date "2023-05-22" @default.
- W4377291234 modified "2023-09-30" @default.
- W4377291234 title "On the Recent Discovery of Coronal [Fe x]λ6374 Emission in the Low-metallicity Dwarf Galaxy SDSS J0944-0038" @default.
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- W4377291234 doi "https://doi.org/10.3847/2515-5172/acd69e" @default.
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