Physics
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..673w&link_type=abstract
The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,
Physics
Scientific paper
It is argued that there is a linear correlation between star formation rate (SFR) and accretion rate for normal bright active galactic nuclei (AGNs). We derive accretion rates for a sample of LINERs (with detected hard X-ray core, a type of LLAGNs) from their hard X-ray luminosities based on spectral calculations for radiatively inefficient accretion flows (RIAFs). We find that LINERs follow the same correlation between SFR and accretion rate defined by normal bright AGNs. It means that the gases feed the black hole and star formation in these low-luminosity LINERs may follow the same way as that in normal bright AGNs, which is roughly consistent with recent numerical simulations on quasar evolution.
Cao Xinwu
Wu Qingwen
No associations
LandOfFree
The Possible Relation between Star Formation Rate and Accretion Rate in Different Types of AGNs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Possible Relation between Star Formation Rate and Accretion Rate in Different Types of AGNs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Possible Relation between Star Formation Rate and Accretion Rate in Different Types of AGNs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-954741