Spatially Resolved Comparison of SFRs from UV and Hα in GASP Gas-stripped Galaxies

Star formation rates (SFRs) in galaxies offer a view of various physical processes across them, and are measured using various tracers, such as H α and ultraviolet (UV). Different physical mechanisms can affect H α and UV emission, resulting in a discrepancy in the corresponding SFR estimates (ΔSFR)...

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מידע ביבליוגרפי

Principais autores:	Neven Tomičić, Ariel Werle, Benedetta Vulcani, Alessandro Ignesti, Alessia Moretti, Anna Wolter, Koshy George, Bianca M. Poggianti, Marco Gullieuszik
פורמט:	Artigo
שפה:	Inglês
יצא לאור:	IOP Publishing 2024-01-01
סדרה:	The Astrophysical Journal
נושאים:	Galaxy clusters Galaxies Interstellar line emission Interstellar line absorption Interstellar medium Star formation
גישה מקוונת:	https://doi.org/10.3847/1538-4357/ad7130
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