The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation
PBN-AR
Instytucja
Wydział Fizyki (Uniwersytet im. Adama Mickiewicza w Poznaniu)
##### Informacje podstawowe
Główny język publikacji
en
Czasopismo
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (35pkt w roku publikacji)
ISSN
0035-8711
EISSN
1365-2966
Wydawca
WILEY-BLACKWELL
DOI
URL
Rok publikacji
2017
Numer zeszytu
Strony od-do
2221-2240
Numer tomu
472
Identyfikator DOI
Liczba arkuszy
##### Autorzy
(liczba autorów: 18)
##### Słowa kluczowe
en
galaxies: active
galaxies: evolution
quasars: general
galaxies: star formation
##### Streszczenia
Język
en
Treść
We investigate the mean star formation rates (SFRs) in the host galaxies of ∼3000 optically selected quasi-stellar objects (QSOs) from the Sloan Digital Sky Survey within the Herschel-ATLAS fields, and a radio-luminous subsample covering the redshift range of z = 0.2-2.5. Using Wide-field Infrared Survey Explorer (WISE) and Herschel photometry (12-500 μm) we construct composite spectral energy distributions (SEDs) in bins of redshift and active galactic nucleus (AGN) luminosity. We perform SED fitting to measure the mean infrared luminosity due to star formation, removing the contamination from AGN emission. We find that the mean SFRs show a weak positive trend with increasing AGN luminosity. However, we demonstrate that the observed trend could be due to an increase in black hole (BH) mass (and a consequent increase of inferred stellar mass) with increasing AGN luminosity. We compare to a sample of X-ray selected AGN and find that the two populations have consistent mean SFRs when matched in AGN luminosity and redshift. On the basis of the available virial BH masses, and the evolving BH mass to stellar mass relationship, we find that the mean SFRs of our QSO sample are consistent with those of main sequence star-forming galaxies. Similarly the radio-luminous QSOs have mean SFRs that are consistent with both the overall QSO sample and with star-forming galaxies on the main sequence. In conclusion, on average QSOs reside on the main sequence of star-forming galaxies, and the observed positive trend between the mean SFRs and AGN luminosity can be attributed to BH mass and redshift dependencies.
ORIGINAL_ARTICLE
##### Inne
System-identifier
857645
Crossref
###### Cytowania
Liczba prac cytujących tę pracę
Brak danych
###### Referencje
Liczba prac cytowanych przez tę pracę
Brak danych