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Cited article:

Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries

Silvia Martínez-Núñez, Peter Kretschmar, Enrico Bozzo, et al.
Space Science Reviews 212 (1-2) 59 (2017)
https://doi.org/10.1007/s11214-017-0340-1

Exploration of spin-down rate of neutron stars in high-mass X-ray binaries

Hai-Lang Dai, Xi-Wei Liu and Xiang-Dong Li
Monthly Notices of the Royal Astronomical Society 457 (4) 3889 (2016)
https://doi.org/10.1093/mnras/stw111

The nature of the X-ray pulsar in M 31: An intermediate-mass X-ray binary?

Shigeyuki Karino
Publications of the Astronomical Society of Japan 68 (6) (2016)
https://doi.org/10.1093/pasj/psw084

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

The evolution of isolated neutron stars until accretion: the role of the initial magnetic field

P. A. Boldin and S. B. Popov
Monthly Notices of the Royal Astronomical Society 407 (2) 1090 (2010)
https://doi.org/10.1111/j.1365-2966.2010.16910.x

Are There Magnetars in High‐Mass X‐Ray Binaries? The Case of Supergiant Fast X‐Ray Transients

E. Bozzo, M. Falanga and L. Stella
The Astrophysical Journal 683 (2) 1031 (2008)
https://doi.org/10.1086/589990

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

Can Thin Disks Produce Anomalous X‐Ray Pulsars?

K. Yavuz Ekşı and M. Alİ Alpar
The Astrophysical Journal 599 (1) 450 (2003)
https://doi.org/10.1086/379193