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Extending the correlation of LRLX to gamma-ray bursts

Jing Lü, Jing-Wen Xing, Yuan-Chuan Zou, Wei-Hua Lei, Qing-Wen Wu, Ding-Xiong Wang


The well-known correlation between radio luminosity (LR) and X-ray luminosity (LX), LR /LX≈10−5, holds for a variety of objects, such as active galactic nuclei, Galactic black holes, solar flares and cool stars. Here we extend the relation to gamma-ray bursts (GRBs) and find that the GRBs also obey a similar LRLX relation, with a slightly different slope of LRLX1.1. This relation implies that the explosions that occur on different scales may have a common underlying origin.


gamma-ray bursts: general — quasars: general — stars: black holes

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Print ISSN: 1674-4527

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