THE XMM-NEWTON /EPIC X-RAY LIGHT CURVE ANALYSIS OF WR 6
We obtained four pointings of over 100 ks each of the well-studied Wolf-Rayet star WR 6 with the XMM-Newton satellite. With a first paper emphasizing the results of spectral analysis, this follow-up highlights the X-ray variability clearly detected in all four pointings. However, phased light curves...
Main Authors: | , , , , , , |
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Format: | Article |
Language: | English |
Published: |
Institute of Physics/American Astronomical Society,
2015-02-04T18:54:04Z.
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Subjects: | |
Online Access: | Get fulltext |
Summary: | We obtained four pointings of over 100 ks each of the well-studied Wolf-Rayet star WR 6 with the XMM-Newton satellite. With a first paper emphasizing the results of spectral analysis, this follow-up highlights the X-ray variability clearly detected in all four pointings. However, phased light curves fail to confirm obvious cyclic behavior on the well-established 3.766 day period widely found at longer wavelengths. The data are of such quality that we were able to conduct a search for event clustering in the arrival times of X-ray photons. However, we fail to detect any such clustering. One possibility is that X-rays are generated in a stationary shock structure. In this context we favor a corotating interaction region (CIR) and present a phenomenological model for X-rays from a CIR structure. We show that a CIR has the potential to account simultaneously for the X-ray variability and constraints provided by the spectral analysis. Ultimately, the viability of the CIR model will require both intermittent long-term X-ray monitoring of WR 6 and better physical models of CIR X-ray production at large radii in stellar winds. United States. National Aeronautics and Space Administration (Smithsonian Astrophysical Observatory contract SV3-73016, Chandra X-Ray Center and Science Instruments) German Aerospace Center (DLR) (grant 50 OR 1302) |
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