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Dynamo generated magnetic configurations in accretion discs and the nature of quasi-periodic oscillations in accreting binary systems
Moss D., Sokoloff D., Suleimanov V.
© ESO 2016.Context. Magnetic fields are important for accretion disc structure. Magnetic fields
Ultraluminous X-ray sources as neutrino pulsars
. The classical limit on the accretion luminosity of a neutron star is given by the Eddington luminosity
Dynamo generated magnetic configurations in accretion discs and the nature of quasi-periodic oscillations in accreting binary systems
Moss D., Sokoloff D., Suleimanov V.
© ESO 2016.Context. Magnetic fields are important for accretion disc structure. Magnetic fields
Radial dependences of physical parameters in α-disk as a consequence of two vertical structure solutions
Lipunova G., Suleimanov V.
Accretion
Propeller effect in action in the ultraluminous accreting magnetar M82 X-2
Tsygankov S., Mushtukov A., Suleimanov V., Poutanen J.
in an accreting neutron star in binary System-The first pulsating ultraluminous X-Ray source X-2 in the galaxy M82
Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disks
Revnivtsev M., Burenin R., Bikmaev I., Kniazev A., Buckley D., Pretorius M., Khamitov I., Ak T., Eker Z., Melnikov S., Crawford S., Pavlinsky M.
asynchronous accreting white dwarfs, XSS J00564+4548, IGR J00234+6141, DO Dra, V1223 Sgr, IGR J15094-6649, IGR
On the nature of pulse profile variations and timing noise in accreting millisecond pulsars
Poutanen J., Ibragimov A., Annala M.
Timing noise in the data on accretion-powered millisecond pulsars (AMP) appears as irregular pulse
On the spreading layer emission in luminous accreting neutron stars
Revnivtsev M., Suleimanov V., Poutanen J.
of luminous accreting neutron stars, the emission of their surfaces is hard to disentangle from their time
Propeller effect in action in the ultraluminous accreting magnetar M82 X-2
Tsygankov S., Mushtukov A., Suleimanov V., Poutanen J.
in an accreting neutron star in binary System-The first pulsating ultraluminous X-Ray source X-2 in the galaxy M82
The impact of neutron star spin on X-ray spectra
of nine NSs for which the spins have been measured that are not accreting pulsars (for which the accretion

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