The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types
Ilse De Looze(Ghent University Hospital), E. Sturm(Max Planck Institute for Extraterrestrial Physics)
Cited by 454
Related Papers
Ionized outflows in local luminous AGN: what are the real densities and outflow rates?
|Monthly Notices of the Royal Astronomical Society|2020|147
Molecular outflows in local galaxies: Method comparison and a role of intermittent AGN driving
|Springer Link (Chiba Institute of Technology)|2020|114
An image of the dust sublimation region in the nucleus of NGC 1068
|Astronomy and Astrophysics|2019|112
The multiphase gas structure and kinematics in the circumnuclear region of NGC 5728
|Monthly Notices of the Royal Astronomical Society|2019|98
LLAMA: normal star formation efficiencies of molecular gas in the centres of luminous Seyfert galaxies
|Monthly Notices of the Royal Astronomical Society|2017|83