Reanalysis of high-resolution XMM-Newton data of V2491 Cygni using models of collisionally ionized hot absorbers

Published January 1, 2017 | Version v1

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Aims. We model spectral absorption features in data of the high-resolution XMM-Newton Reflection Grating Spectrometer.

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March 15, 2021

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Journal article

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ASTRONOMY & ASTROPHYSICS, 598, 2017.

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Creative Commons Attribution 4.0 International

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