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1887
3561915
Physics of ULIRGs with MUSE and ALMA: the PUMA project. IV. No tight relation between cold molecular outflow rates and AGN luminosities
Author(s):
Lamperti, I.; Pereira-Santaella, M.; Perna, M.; Colina, L.; Arribas, S.; García-Burillo, S.; González-Alfonso, E.; Aalto, S.; Alonso-Herrero, A.; Combes, F.; Labiano, A.; Piqueras-López, J.; Rigopoulou, D.; Werf, P.P. van der (
0000-0002-4389-832x
)
Published
2022
Publication type
Article / Letter to editor
galaxies evolution
galaxies nuclei
galaxies active
galaxies starburst
Astrophysics - Astrophysics of Galaxies
Date issued
2022
Language
English
Is part of
Astronomy & Astrophysics (2022), A45
hdl
1887/3561915
doi
10.1051/0004-6361/202244054
URL
https://ui.adsabs.harvard.edu/abs/2022A&A...668A..45L
Persistent identifier url
https://hdl.handle.net/1887/3561915
Documents
01 - Astronomy_and_Astrophysics_668_2022_A45
version: Publisher's Version
Full text at Publisher's site
Open Access