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Luminosity and colors of the early optical transient of GRB060218 in the context of the optical afterglows

机译:GRB060218在光学余量的背景下的早期光学瞬态的亮度和颜色

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We investigate the luminosity and colors of the optical afterglow (OA) of GRB060218 during t — To < 2 days in the context of the OAs of long GRBs. The R-band absolute magnitude —19.5 at (t -To)_(rest) = 1.5 d places this event below or at the lower end of the statistical distribution of the spectrally homogeneous ensemble of 23 OAs of long GRBs which we considered in our previous work [13, 14]. We find that the color indices of this phase are not consistent with those of the ensemble of OAs of GRBs, but their time evolution is. No variations of reddening even in the initial phase of these OAs are present. We argue that the optical and UV emission is not a simple continuation (Rayleigh-Jeans tail) of the X-ray emission.We also show that although both GRB060218 and XRF030723 possess a very soft gamma-ray spectrum, sorting them to X-ray flashes, the color indices of their early OAs are mutually discordant.
机译:我们在长GRBS的OA的背景下研究了GB060218期间GRB060218的光学余量(OA)的光度和颜色。 R带绝对幅度-19.5在(t-to)_(休息)= 1.5 d下面或在我们考虑的长GRBS的谱分布的统计分布的统计分布的统计分布下端的下端以前的工作[13,14]。我们发现,此阶段的颜色指数与GRBS OAS的集合的颜色指数不一致,但它们的时间进化是。即使在这些OA的初始阶段也没有变红的变化。我们认为光学和紫外线排放不是X射线发射的简单延续(瑞利牛仔裤尾部)。我们还表明GRB060218和XRF030723都具有非常软的伽马射线光谱,将它们分类为X射线闪烁,他们早期OA的颜色指数相互不和谐。

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