SRG/ART-XC, Swift, NICER, and NuSTAR study of different states of the transient X-ray pulsar MAXI J0903-531

Tsygankov, S.S.; Molkov, S.V.; Doroshenko, V.; Mushtukov, A.; Mereminskiy, I.A.; Semena, A.N.; ... ; Lutovinov, A.A. (2022)

Article / Letter to editor

• Accretion
• Accretion disks
• Magnetic fields
• X-rays - binaries
• Stars - neutron
• Pulsars - individual - MAXI J0903-531
• Radiative transfer
• Astrophysics - high energy astrophysical phenomena

• All authors: Tsygankov, S.S.; Molkov, S.V.; Doroshenko, V.; Mushtukov, A.; Mereminskiy, I.A.; Semena, A.N.; Thalhammer, P.; Wilms, J.; Lutovinov, A.A.
• Date: 2022
• Journal: Astronomy & Astrophysics
• Volume: 661
• DOI: doi:10.1051/0004-6361/202141821
• Link: https://ui.adsabs.harvard.edu/abs/2022A&A...661A..45T