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Home All issues A&A, 404 3 (2003) 1023-1032 Article references

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Cited article:

Cyclical accretion regime change in the slow X-ray pulsar 4U 0114+65 observed with Chandra

G. Sanjurjo-Ferrín, J. M. Torrejón, K. Postnov, M. Nowak, J. J. Rodes-Roca, L. Oskinova, J. Planelles-Villalva and N. Schulz
Astronomy & Astrophysics 694 A192 (2025)
https://doi.org/10.1051/0004-6361/202452789

Magnetic Inclination Evolution of Accreting Neutron Stars in Intermediate/Low-mass X-Ray Binaries

Hao-ran Yang and Xiang-dong Li
The Astrophysical Journal 945 (1) 2 (2023)
https://doi.org/10.3847/1538-4357/acba09

Timing Properties of the X-Ray Accreting Pulsar 1A 0535+262 Studied with Insight-HXMT

P. J. Wang, L. D. Kong, S. Zhang, V. Doroshenko, A. Santangelo, L. Ji, E. S. Yorgancioglu, Y. P. Chen, S. N. Zhang, J. L. Qu, M. Y. Ge, J. Li, Z. Chang, L. Tao, J. Q. Peng and Q. C. Shui
The Astrophysical Journal 935 (2) 125 (2022)
https://doi.org/10.3847/1538-4357/ac8230

Revisiting the spectral and timing properties of 4U 1909+07 with NuSTAR and Astrosat

Gaurava K Jaisawal, Sachindra Naik, Wynn C G Ho, et al.
Monthly Notices of the Royal Astronomical Society 498 (4) 4830 (2020)
https://doi.org/10.1093/mnras/staa2604

Constraining compactness and magnetic field geometry of X-ray pulsars from the statistics of their pulse profiles

M. Annala and J. Poutanen
Astronomy and Astrophysics 520 A76 (2010)
https://doi.org/10.1051/0004-6361/200912773

Timing characteristics of the hard X-ray emission from bright X-ray pulsars based on INTEGRAL data

A. A. Lutovinov and S. S. Tsygankov
Astronomy Letters 35 (7) 433 (2009)
https://doi.org/10.1134/S1063773709070019

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

The Electromagnetic Spectrum of Neutron Stars

Altan Baykal
NATO Science Series II. Mathematics, Physics and Chemistry, The Electromagnetic Spectrum of Neutron Stars 210 263 (2005)
https://doi.org/10.1007/1-4020-3861-5_26