{ "id": "1708.08203", "version": "v1", "published": "2017-08-28T06:28:23.000Z", "updated": "2017-08-28T06:28:23.000Z", "title": "The correlations of multi-wave band luminosity and BLR luminosity in Fermi 2LAC blazars", "authors": [ "Zerui Wang", "Rui Xue", "Zhaohua Xie", "Leiming Du", "Tingfeng Yi", "Yunbing Xu", "Wenguang Liu" ], "comment": "10 pages, 1 figure, accepted for publication in Ap&SS", "categories": [ "astro-ph.HE" ], "abstract": "We collect a sample of 78 Fermi detected blazars with broad line region (BLR) data and the quasi-simultaneous multi-wave band data. By analyzing the sample, we find: (1) For whole blazar sample, there exist significant correlations between radio, $\\gamma$-ray luminosity and BLR luminosity. The slope of the best-fit linear regression equation is close to the theoretical value 1. Our results provided another support of jet-disk symbiosis. (2) For FSRQ sample, we find a significant correlation between radio luminosity and optical luminosity, and weaker correlations between X-ray luminosity and radio, optical luminosity. It indicates that the X-ray band radiation mechanism is slightly different from radio and optical bands. The X-ray emission is diluted by inverse Compton scattering (IC). There is a significant correlation between BLR luminosity and $\\gamma$-ray luminosity, but no correlations between X-ray luminosity and BLR, $\\gamma$-ray luminosity, which suggests that the seed soft photons are different for IC process. From these results we suggest that the X-ray band emission is diluted by synchrotron self-Compton (SSC) process, $\\gamma$-ray band emission is produced by external Compton (EC) process.", "revisions": [ { "version": "v1", "updated": "2017-08-28T06:28:23.000Z" } ], "analyses": { "keywords": [ "multi-wave band luminosity", "blr luminosity", "fermi 2lac blazars", "significant correlation", "ray luminosity" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable" } } }