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Infrared Point-Source Variability between the Spitzer and Midcourse Space Experiment Surveys of the Galactic Midplane

机译:银河中平面的斯皮策和中途空间实验测量之间的红外点源变异

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We present a list of 552 sources with suspected variability, based on a comparison of mid-infrared photometry from the GLIMPSE I and Midcourse Space Experiment (MSX) surveys, which were carried out nearly a decade apart. We were careful to address issues such as the difference in resolution and sensitivity between the two surveys, as well as the differences in the spectral responses of the instruments. We selected only sources where the IRAC 8.0 μm and MSX 8.28 μm fluxes differ by more than a factor of 2, in order to minimize contamination from sources where the difference in fluxes at 8 μm is due to a strong 10 μm silicate feature. We present a subset of 40 sources for which additional evidence suggests variability, using 2MASS and MIPSGAL data. Based on a comparison with the variability flags in the IRAS and MSX point-source catalogs we estimate that at least a quarter of the 552 sources and at least half of the 40 sources in the subset are truly variable. In addition, we tentatively confirm the variability of one source using multiepoch IRAS LRS spectra. We suggest that most of the sources in our list are likely to be asymptotic giant branch stars.
机译:根据GLIMPSE I和中途空间实验(MSX)调查中距离红外光度法的比较,我们列出了552个可疑变异源的清单,这两个距离相隔近十年。我们小心地解决了诸如两次测量之间的分辨率和灵敏度差异以及仪器的光谱响应差异之类的问题。我们仅选择IRAC 8.0μm和MSX 8.28μm通量相差大于2的源,以最大程度地减少源于8μm通量差异归因于强大的10μm硅酸盐特征的污染。我们使用2MASS和MIPSGAL数据,提供了40个来源的子集,其更多的证据表明了变异性。根据与IRAS和MSX点源目录中的可变性标记的比较,我们估计该子集中552个源中至少有四分之一和40个源中至少有一半是真正可变的。此外,我们使用多时期IRAS LRS光谱初步确定了一种来源的变异性。我们建议清单中的大多数来源可能都是渐近的巨型分支恒星。

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