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- W2121494879 abstract "We present evidence for excess long-wavelength emission from two high-mass X-ray binaries, IGR J16318-4848 and GX 301-2, that show enormous obscuration (NH ≃ 1023-1024 cm-2) in their X-ray spectra. Using archival near- and mid-infrared data, we show that the spectral energy distributions of IGR J16318-4848 and GX 301-2 are substantially higher in the mid-infrared than their expected stellar emission. We successfully fit the excesses with ~1000 K blackbodies, which suggests that they are due to warm circumstellar dust that also gives rise to the X-ray absorption. However, we need further observations to constrain the detailed properties of the excesses. This discovery highlights the importance of mid-infrared observations for understanding highly obscured X-ray binaries." @default.
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- W2121494879 date "2006-09-13" @default.
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- W2121494879 title "Long-Wavelength Excesses in Two Highly Obscured High-Mass X-Ray Binaries: IGR J16318-4848 and GX 301-2" @default.
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- W2121494879 doi "https://doi.org/10.1086/508369" @default.
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