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X-ray Observations of Historical Classical Nova Counterparts with eROSITA Telescope Onboard the SRG Orbital Observatory during the All-Sky Survey
Galiullin I.I., Gilfanov M.R.
Abstract: The X-ray emission from the counterparts of historical classical novae (CNe) in our
Study of the relation between the jet and accretion-disk emission in Blazars using RATAN-600 multifrequency data
Mufakharov T., Sotnikova Y., Erkenov A., Mingaliev M.
results are consistent with the theoretical predictions about the close relationship of the accretion disk
Study of the relation between the jet and accretion-disk emission in Blazars using RATAN-600 multifrequency data
Mufakharov T., Sotnikova Y., Erkenov A., Mingaliev M.
results are consistent with the theoretical predictions about the close relationship of the accretion disk
NuSTAR and Swift Observations of the Ultraluminous X-Ray Source IC 342 X-1 in 2016: Witnessing Spectral Evolution
Shidatsu M., Ueda Y., Fabrika S.
-luminosity state of IC 342 X-1. The observed spectrum has a broader profile than the multi-color disk blackbody
Modelling nova populations in galaxies
Chen H., Woods T., Yungelson L., Gilfanov M., Han Z.
© 2016 The Authors.Theoretical modelling of the evolution of classical and recurrent novae plays
Influence of Compton scattering on the broad-band X-ray spectra of intermediate polars
Suleimanov V., Poutanen J., Falanga M., Werner K.
are intermediate polars where the magnetic field is strong enough to channel the accreting matter to the magnetic
Photometric and spectral studies of the eclipsing polar CRTS CSS081231 J071126+440405
Borisov N., Gabdeev M., Shimansky V., Katysheva N., Kolbin A., Shugarov S., Goranskij V.
shown a shift of the emission line-forming region along the accretion stream closer to the white dwarf
Ultraluminous X-ray sources as neutrino pulsars
. The classical limit on the accretion luminosity of a neutron star is given by the Eddington luminosity
Ultraluminous X-ray sources with flat-topped noise and QPO
Atapin K., Fabrika S., Caballero-García M.
variability is the mass accretion rate that varies ≳3 between different observations of the same source
Modelling nova populations in galaxies
Chen H., Woods T., Yungelson L., Gilfanov M., Han Z.
© 2016 The Authors.Theoretical modelling of the evolution of classical and recurrent novae plays

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