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)...

詳細記述

書誌詳細

主要な著者:	Neven Tomičić, Ariel Werle, Benedetta Vulcani, Alessandro Ignesti, Alessia Moretti, Anna Wolter, Koshy George, Bianca M. Poggianti, Marco Gullieuszik
フォーマット:	Artigo
言語:	Inglês
出版事項:	IOP Publishing 2024-01-01
シリーズ:	The Astrophysical Journal
主題:	Galaxy clusters Galaxies Interstellar line emission Interstellar line absorption Interstellar medium Star formation
オンライン･アクセス:	https://doi.org/10.3847/1538-4357/ad7130
タグ:	タグ追加 タグなし, このレコードへの初めてのタグを付けませんか!