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Cited article:

Monitoring clumpy wind accretion in supergiant fast-X-ray transients with XMM-Newton

C. Ferrigno, E. Bozzo, P. Romano

A&A, 642 (2020) A73

Published online: 2020-10-06

DOI: https://doi.org/10.1051/0004-6361/202038278

This article has been cited by the following article(s):

NuSTAR and Swift observations of two supergiant fast X-ray transients: AX J1841.0−0536 and SAX J1818.6−1703

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Swift, NuSTAR, and INTEGRAL observations of the symbiotic X-ray binary IGR J16194-2810

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XMM-Newton and Swift observations of supergiant high mass X-ray binaries

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The symbiotic X-ray binaries Sct X-1, 4U 1700+24, and IGR J17329−2731

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Accretion of a clumped wind from a red supergiant donor on to a magnetar is suggested by the analysis of the XMM–Newton and NuSTAR observations of the X-ray binary 3A 1954+319

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Color–color diagrams as tools for assessment of the variable absorption in high mass X-ray binaries

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Radiography in high mass X-ray binaries

I. El Mellah, V. Grinberg, J. O. Sundqvist, F. A. Driessen and M. A. Leutenegger
Astronomy & Astrophysics 643 A9 (2020)
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