The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift
Research output: Contribution to journal › Journal article › Research › peer-review
We exploit the recent, wide samples of far-infrared (FIR) selected
galaxies followed up in X-rays and of X-ray/optically selected active
galactic nuclei (AGNs) followed up in the FIR band, along with the
classic data on AGNs and stellar luminosity functions at high redshift z
>~ 1.5, to probe different stages in the coevolution of supermassive
black holes (BHs) and host galaxies. The results of our analysis
indicate the following scenario: (1) the star formation in the host
galaxy proceeds within a heavily dust-enshrouded medium at an almost
constant rate over a timescale
Original language | English |
---|---|
Article number | 69 |
Journal | Astrophysical Journal |
Volume | 782 |
Issue number | 2 |
Number of pages | 25 |
ISSN | 0004-637X |
DOIs | |
Publication status | Published - 1 Feb 2014 |
Externally published | Yes |
- galaxies: elliptical and lenticular, cD, galaxies: evolution, galaxies: formation, galaxies: high-redshift, quasars: general
Research areas
ID: 230475393