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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
Multiwavelength observations reveal a faint candidate black hole X-ray binary in IGR J17285−2922
M Stoop, J van den Eijnden, N Degenaar, et al. Monthly Notices of the Royal Astronomical Society 507(1) 330 (2021) https://doi.org/10.1093/mnras/stab2127
The M Supergiant High-mass X-Ray Binary 4U 1954+31
Kenneth H. Hinkle, Thomas Lebzelter, Francis C. Fekel, Oscar Straniero, Richard R. Joyce, Lisa Prato, Nicole Karnath and Nolan Habel The Astrophysical Journal 904(2) 143 (2020) https://doi.org/10.3847/1538-4357/abbe01
A Census of Symbiotic Stars in the 2MASS,
WISE
, and
Gaia
Surveys
Stavros Akras, Lizette Guzman-Ramirez, Marcelo L. Leal-Ferreira and Gerardo Ramos-Larios The Astrophysical Journal Supplement Series 240(2) 21 (2019) https://doi.org/10.3847/1538-4365/aaf88c
Periodic signals from the Circinus region: two new cataclysmic variables and the ultraluminous X-ray source candidate GC X-1
P. Esposito, G. L. Israel, D. Milisavljevic, et al. Monthly Notices of the Royal Astronomical Society 452(2) 1112 (2015) https://doi.org/10.1093/mnras/stv1379
SPECTRAL AND TIMING NATURE OF THE SYMBIOTIC X-RAY BINARY 4U 1954+319: THE SLOWEST ROTATING NEUTRON STAR IN AN X-RAY BINARY SYSTEM
Randall K. Smith, Richard Mushotzky, Koji Mukai, Tim Kallman, Craig B. Markwardt and Jack Tueller Publications of the Astronomical Society of Japan 60(sp1) S43 (2008) https://doi.org/10.1093/pasj/60.sp1.S43
A Comparison of the Variability of the Symbiotic X‐Ray Binaries GX 1+4, 4U 1954+31, and 4U 1700+24 fromSwiftBAT andRXTEASM Observations
R. H. D. Corbet, J. L. Sokoloski, K. Mukai, C. B. Markwardt and J. Tueller The Astrophysical Journal 675(2) 1424 (2008) https://doi.org/10.1086/526337
INTEGRAL long-term monitoring of the supergiant fast X-ray transient XTE J1739-302