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

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2017-02-01

Author

Balman, Şölen
Gamsizkan, C.

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

Subject Keywords

X-rays: stars, Stars: individual: V2491 Cyg, Binaries: general, Novae, cataclysmic variables, Stars: abundances, Stars: winds, outflows

URI

https://hdl.handle.net/11511/57268

Journal

ASTRONOMY & ASTROPHYSICS

DOI

https://doi.org/10.1051/0004-6361/201629360

Collections

Department of Physics, Article

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Citation Formats

Ş. Balman and C. Gamsizkan, “Reanalysis of high-resolution XMM-Newton data of V2491 Cygni using models of collisionally ionized hot absorbers,” ASTRONOMY & ASTROPHYSICS, pp. 0–0, 2017, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/57268.