Measuring 60 pc-scale Star Formation Rate of the Nearby Seyfert Galaxy NGC 1068 with ALMA, HST, VLT/MUSE, and VLA

Measuring 60 pc-scale Star Formation Rate of the Nearby Seyfert Galaxy NGC 1068 with ALMA, HST, VLT/MUSE, and VLA

The star formation rate (SFR) is a fundamental parameter for describing galaxies and inferring their evolutionary course. H ii regions yield the best measure of instantaneous SFR in galaxies, although the derived SFR can have large uncertainties depending on tracers and assumptions. We present an SF...

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Autors principals: Yuzuki Nagashima, Toshiki Saito, Soh Ikarashi, Shuro Takano, Kouichiro Nakanishi, Nanase Harada, Taku Nakajima, Akio Taniguchi, Tomoka Tosaki, Kazuharu Bamba
Format: Article
Idioma:English
Publicat: IOP Publishing 2024-01-01
Col·lecció:The Astrophysical Journal
Matèries:
Galaxy evolution
H II regions
Radio astronomy
Seyfert galaxies
Star formation
Accés en línia:https://doi.org/10.3847/1538-4357/ad6312

Internet

https://doi.org/10.3847/1538-4357/ad6312

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