{ "id": "1104.3235", "version": "v1", "published": "2011-04-16T12:28:45.000Z", "updated": "2011-04-16T12:28:45.000Z", "title": "Evidence for Rapidly Rotating Black Holes in FR I Radio Galaxies", "authors": [ "Qingwen Wu", "Xinwu Cao", "Ding-Xiong Wang" ], "comment": "Accepted by ApJ", "categories": [ "astro-ph.HE" ], "abstract": "We investigate the correlation between 151 MHz radio luminosity, L_151MHz, and jet power, P_jet, for a sample of low-power radio galaxies, of which the jet power is estimated from X-ray cavities. The jet power for a sample of FR I radio galaxies is estimated with the derived empirical correlation. We find that P_jet/L_Edd is positively correlated with Lx(2-10 keV)/L_Edd for FR Is, where L_Edd is the Eddington luminosity and Lx(2-10 keV) is 2-10 keV X-ray luminosity. We calculate the jet power of a hybrid model, as a variant of Blandford-Znajek model proposed by Meier, based on the global solution of the advection-dominated accretion flow (ADAF) surrounding a Kerr black hole (BH). Our model calculations suggest that the maximal jet power is a function of mass accretion rate and the black hole spin parameter j. The hard X-ray emission is believed to be mainly from the ADAFs in FR Is, and the mass accretion rate is therefore constrained with the X-ray emission in our ADAF model calculations. We find that the dimensionless angular momentum of BH j>~0.9 is required in order to reproduce the observed relation of P_jet/L_Edd-Lx(2-10 keV)/L_Edd for FR Is. Our conclusion will be strengthened if part of the X-ray emission is contributed by the jets. Our results suggest that BHs in FR I radio galaxies are rapidly spinning, which are almost not affected by the uncertainty of the black hole mass estimates.", "revisions": [ { "version": "v1", "updated": "2011-04-16T12:28:45.000Z" } ], "analyses": { "keywords": [ "rapidly rotating black holes", "radio galaxies", "jet power", "x-ray emission", "mass accretion rate" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/735/1/50", "journal": "The Astrophysical Journal", "year": 2011, "month": "Jul", "volume": 735, "number": 1, "pages": 50 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 896505, "adsabs": "2011ApJ...735...50W" } } }