Extending the correlation of LR - LX to gamma-ray bursts

Extending the correlation of LR - LX to gamma-ray bursts

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...

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Veröffentlicht in:天文和天体物理学研究：英文版 2015-05 (5), p.617-622
1. Verfasser: Jing Lu Jing-Wen Xing Yuan-Chuan Zou Wei-Hua Lei Qing-Wen Wu Ding-Xiong Wang
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Sprache:eng
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X射线
伽玛射线爆发
伽马射线暴
光度
太阳耀斑
无线电
活动星系核
黑洞
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creator Jing Lu Jing-Wen Xing Yuan-Chuan Zou Wei-Hua Lei Qing-Wen Wu Ding-Xiong Wang
description 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 LR - LX relation, with a slightly different slope of LR ∝ LX^1.1. This relation implies that the explosions that occur on different scales may have a common underlying origin.
doi_str_mv 10.1088/1674-4527/15/5/001
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subjects X射线
伽玛射线爆发
伽马射线暴
光度
太阳耀斑
无线电
活动星系核
黑洞
title Extending the correlation of LR - LX to gamma-ray bursts
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