arXiv Analytics

Sign in

arXiv:2003.13487 [astro-ph.GA]AbstractReferencesReviewsResources

Accretion rate in AGN and X-ray-to-optical flux ratio at z $\le$ 0.2

Asrate Gaulle, Mirjana Pović, Dejene Zewdie

Published 2020-03-30Version 1

We explored a sample of 545 local galaxies using data from the 3XMM-DR7 and SDSS-DR8 surveys. We carried out all analyses up to z\,$\sim$\,0.2, and we studied the relation between X/O flux ratio and accretion rate for different classes of active galaxies such as LINERs and Seyfert 2. We obtained a slight correlation between the two parameters if the whole sample of AGN is used. However, LINERs and Sy2 galaxies show different properties, slight correlation and slight anti-correlation, respectively. This could confirm that LINERs and Sy2 galaxies have different accretion efficiencies and maybe different accretion disc properties,as has been suggested previously. Keywords: galaxies - active; AGN - accretion rate; AGN - black hole masses; AGN - X-ray properties; AGN - optical properties

Comments: 3 page, 4 figures, Proceedings paper of the IAU symposium "Nuclear Activity in Galaxies Across Cosmic Time" (Ethiopia) accepted to be published under the Cambridge University Press, eds. M. Povic, P. Marziani, J. Masegosa, H. Netzer, S. H. Negu, and S. B. Tessema
Categories: astro-ph.GA
Related articles: Most relevant | Search more
arXiv:2306.02494 [astro-ph.GA] (Published 2023-06-04)
Comparative tests of accretion rates of quasars derived using a new empirical and an existing theoretical relation: Insights into black hole properties and growth
arXiv:1411.7388 [astro-ph.GA] (Published 2014-11-26)
Black-hole masses, accretion rates and hot- and cold-mode accretion in radio galaxies at z~1
arXiv:2309.15898 [astro-ph.GA] (Published 2023-09-27)
Three regimes of black hole feedback