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Cited article:

The First High-contrast Images of Near High-mass X-Ray Binaries with Keck/NIRC2

M. Prasow-Émond, J. Hlavacek-Larrondo, K. Fogarty, É. Artigau, D. Mawet, P. Gandhi, J. F. Steiner, J. Rameau, D. Lafrenière, A. Fabian, D. J. Walton, R. Doyon and B. B. 彬 Ren 任
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A new radio census of neutron star X-ray binaries

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Monthly Notices of the Royal Astronomical Society 507 (3) 3899 (2021)
https://doi.org/10.1093/mnras/stab1995

NuSTAR rules out a cyclotron line in the accreting magnetar candidate 4U2206+54

J M Torrejón, P Reig, F Fürst, et al.
Monthly Notices of the Royal Astronomical Society 479 (3) 3366 (2018)
https://doi.org/10.1093/mnras/sty1628

An XMM-Newton and NuSTAR Study of IGR J18214-1318: A Non-pulsating High-mass X-Ray Binary with a Neutron Star

Francesca M. Fornasini, John A. Tomsick, Matteo Bachetti, Roman A. Krivonos, Felix Fürst, Lorenzo Natalucci, Katja Pottschmidt and Jörn Wilms
The Astrophysical Journal 841 (1) 35 (2017)
https://doi.org/10.3847/1538-4357/aa6ff4

High-mass X-ray binaries in the Milky Way

Roland Walter, Alexander A. Lutovinov, Enrico Bozzo and Sergey S. Tsygankov
The Astronomy and Astrophysics Review 23 (1) (2015)
https://doi.org/10.1007/s00159-015-0082-6

AN ACCRETION MODEL FOR THE ANOMALOUS X-RAY PULSAR 4U 0142+61

J. E. Trümper, K. Dennerl, N. D. Kylafis, Ü. Ertan and A. Zezas
The Astrophysical Journal 764 (1) 49 (2013)
https://doi.org/10.1088/0004-637X/764/1/49

Spin and spectral variations of a peculiar high-mass X-ray binary 4U 2206+54

Wei Wang
Monthly Notices of the Royal Astronomical Society 432 (2) 954 (2013)
https://doi.org/10.1093/mnras/stt516

Quasi-spherical subsonic accretion in X-ray pulsars

Nikolai I. Shakura, Konstantin A. Postnov, Aleksandra Yu. Kochetkova and Lineya Hjalmarsdotter
Uspekhi Fizicheskih Nauk 183 (4) 337 (2013)
https://doi.org/10.3367/UFNr.0183.201304a.0337

ANXMM-NEWTONSPECTRAL AND TIMING STUDY OF IGR J16207 – 5129: AN OBSCURED AND NON-PULSATING HMXB

John A. Tomsick, Sylvain Chaty, Jerome Rodriguez, et al.
The Astrophysical Journal 694 (1) 344 (2009)
https://doi.org/10.1088/0004-637X/694/1/344

Discovery of slow X-ray pulsations in the high-mass X-ray binary 4U 2206+54

P. Reig, J. M. Torrejón, I. Negueruela, et al.
Astronomy & Astrophysics 494 (3) 1073 (2009)
https://doi.org/10.1051/0004-6361:200810950

Very peculiar wind from BD+53°2790, the optical counterpart to 4U 2206+54

P. Blay, M. Ribó and I. Negueruela
Astrophysics and Space Science 320 (1-3) 145 (2009)
https://doi.org/10.1007/s10509-008-9846-z

INTEGRAL long-term monitoring of the supergiant fast X-ray transient XTE J1739-302

P. Blay, S. Martínez-Núñez, I. Negueruela, et al.
Astronomy & Astrophysics 489 (2) 669 (2008)
https://doi.org/10.1051/0004-6361:200809385

SwiftBAT andRXTEObservations of the Peculiar X‐Ray Binary 4U 2206+54: Disappearance of the 9.6 Day Modulation

R. H. D. Corbet, C. B. Markwardt and J. Tueller
The Astrophysical Journal 655 (1) 458 (2007)
https://doi.org/10.1086/509319

Wind accretion in the massive X-ray binary 4U 2206+54: abnormally slow wind and a moderately eccentric orbit

M. Ribó, I. Negueruela, P. Blay, J. M. Torrejón and P. Reig
Astronomy & Astrophysics 449 (2) 687 (2006)
https://doi.org/10.1051/0004-6361:20054206

Exploration of the \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $P_{s}$ \end{document} ‐ \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2}! \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $P_{\mathrm{orb}\,}$ \end{document} Relation for Wind‐fed X‐Ray Pulsars

Hai‐Lang Dai, Xi‐Wei Liu and Xiang‐Dong Li
The Astrophysical Journal 653 (2) 1410 (2006)
https://doi.org/10.1086/508735

Astrophysics in 2005

Virginia Trimble, Markus J. Aschwanden and Carl J. Hansen
Publications of the Astronomical Society of the Pacific 118 (845) 947 (2006)
https://doi.org/10.1086/506157

Multiwavelength monitoring of BD +53°2790, the optical counterpart to 4U 2206+54

P. Blay, I. Negueruela, P. Reig, et al.
Astronomy & Astrophysics 446 (3) 1095 (2006)
https://doi.org/10.1051/0004-6361:20053951