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...

Полное описание

Библиографические подробности
Главные авторы: Yuzuki Nagashima, Toshiki Saito, Soh Ikarashi, Shuro Takano, Kouichiro Nakanishi, Nanase Harada, Taku Nakajima, Akio Taniguchi, Tomoka Tosaki, Kazuharu Bamba
Формат: Статья
Язык:English
Опубликовано: IOP Publishing 2024-01-01
Серии:The Astrophysical Journal
Предметы:
Galaxy evolution
H II regions
Radio astronomy
Seyfert galaxies
Star formation
Online-ссылка:https://doi.org/10.3847/1538-4357/ad6312

Internet

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

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