Physical Conditions of the Ionized Superwind in NGC 253 with VLT/MUSE

We present an analysis of the H α -emitting ionized gas in the warm phase of the NGC 253 outflow using integral field spectroscopy from the Multi Unit Spectroscopic Explorer. In each spaxel, we decompose H α , [N ii ], and [S ii ] emission lines into a system of up to three Gaussian components, acco...

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Bibliographic Details
Main Authors: Serena A. Cronin, Alberto D. Bolatto, Enrico Congiu, Keaton Donaghue, Kathryn Kreckel, Adam K. Leroy, Rebecca C. Levy, Sylvain Veilleux, Fabian Walter, Lenin Nolasco
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/add738
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