AGN wind scaling relations and the co-evolution of black holes and galaxies
Astronomical Observatory of Rome · National Institute for Astrophysics · +10 more institutions
Indexed inarxivcrossrefdatacitedoaj
Abstract
Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as the main mechanism responsible for regulating star formation in active galactic nucleus (AGN) host galaxies. However, the relationships between AGN activity, radiation, winds, and star formation are complex and still far from being understood.
Citation impact
596
total citations
- FWCI
- 38.19
- Percentile
- 100%
- References
- 290
Citations per year
Authors
17- FFF. FioreCorresponding
Astronomical Observatory of Rome, National Institute for Astrophysics
- CFC. Feruglio
Trieste Astronomical Observatory
- FSFrancesco Shankar
University of Southampton
- MBM. Bischetti
Astronomical Observatory of Rome, National Institute for Astrophysics
- ABA. Bongiorno
Astronomical Observatory of Rome, National Institute for Astrophysics
Topics & keywords
Topics
Keywords
- Physics
- Astrophysics
- Galaxy
- Star formation
- Luminosity
- Astronomy
- Active galactic nucleus
- Stellar mass
No related works found for this paper.
Funding
- NSNational Science FoundationAwards: PP00P2_166159, PP00P2_138979
- ECEuropean CommissionAwards: 321913, 664931, 695671
- SNSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungAwards: PP00P2_138979, 166159, PP00P2, PP00P2_138979 and PP00P2_166159, PP00P2_166159, 138979
- SAScience and Technology Facilities CouncilAwards: ST/K003119/1, 664931, ST/M001172/1, ST/M001326/1, 695671