X-ray AGN fraction increases with central star formation rate density in local galaxies, supporting coeval black hole and galaxy growth with only modest time-averaged AGN feedback effects.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Investigating central star formation in local AGN host galaxies: is there tension between coeval growth and AGN feedback?
X-ray AGN fraction increases with central star formation rate density in local galaxies, supporting coeval black hole and galaxy growth with only modest time-averaged AGN feedback effects.