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The Possible Origins of the VR Magnification Ratios of Q0957+561AB

机译:Q0957 + 561AB的VR倍率比的可能起源

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We present VR magnification ratios of the double quasar Q0957+561AB, which are inferred from frames taken with the 2.56m Nordic Optical Telescope From two different photometric techniques (pho2comC and psfphot) and a reasonable range for the time delay in the system (415-430 days), we find optical continuum ratios depending on the wavelength These chromatic ratios are consistent with either differential extinction in a dust system or gravitational microlensing in the deflector Although the dusty scenario is only viable for a compact dust cloud in the line of sight to the A component, the possible values for the differential extinction and the ratio of total to selective extinction in the V band are surprisingly reasonable. To decide on the true origin of the anomalous ratios (extinction, microlensing or a mixed scenario), we are carrying out new monitoring campaigns and planning detailed observations from the best ground-based and space telescopes
机译:我们呈现双Quasar Q0957 + 561ab的VR倍率率,这些比例由来自256米北欧光学望远镜的帧从两种不同的光度技术(PHO2COMC和PHOF照片)和系统延迟的合理范围(415- 430天),我们发现光学连续统定比率,根据波长,这些色差与灰尘系统中的灰尘系统中的差分灭火一致,尽管尘土飞扬的场景对于视线中的紧凑型尘埃云仅是可行的A组件,差分消光的可能值和V频段中的选择性灭绝的总量令人惊讶地合理。要决定异常比率的真实起源(灭绝,微溶剂或混合情景),我们正在进行新的监控活动和规划来自最佳地面和空间望远镜的详细观察

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