Radio spectra and radio-loudness of low-luminosity AGNs

Details Radio spectra and radio-loudness of low-luminosity AGNs Radio spectra and radio-loudness of low-luminosity AGNs

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..54..335d&link_type=abstract

"Journal of Physics: Conference Series, Volume 54, Proceedings of "The Universe Under the Microscope - Astrophysics at High Angu

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We investigated the empirical relation between black hole mass (mBH), Eddington ratio (Lbol/LEdd), and radio loudness (RRL a ratio of radio to optical luminosity) of nearby low-luminosity active galactic nuclei (LLAGNs). A best-fit plane was found in the three-dimensional space using a sample of 48 nearby LLAGNs: RRL = mBH0.52±0.l4(Lbol/LEdd)-0.39±0.08. This suggests that spectral energy distributions of LLAGNs are controlled by both the black hole mass and accretion rate.

Affiliated with

Also associated with

No associations

Rating

Radio spectra and radio-loudness of low-luminosity 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 Radio spectra and radio-loudness of low-luminosity AGNs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio spectra and radio-loudness of low-luminosity AGNs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1548066