Электронный архив

ПросмотрНаучные публикации в Scopus по теме "X-rays: binaries"

ПросмотрНаучные публикации в Scopus по теме "X-rays: binaries"

Отсортировать по:Сортировать:Результаты поиска на странице:

  • Ibragimov A.; Zdziarski A.; Poutanen J. (2007)
    We study theoretical interpretations of the ∼150-d (superorbital) modulation observed in X-ray and radio emission of Cyg X-1 in the framework of models connecting this phenomenon to precession. Precession changes the ...
  • Poutanen J.; Zdziarski A.; Ibragimov A. (2008)
    We discover a pronounced dependence of the strength of the soft X-ray orbital modulation and the spectral hardness in Cyg X-1 in the hard state on its superorbital phase. We find, our results can be well modelled as a ...
  • Неизвестный автор (2018)
    © 2017 The Author(s). GS 1826-238 is a well-studied low-mass X-ray binary neutron star. This source was in a persistent hard state since its discovery in 1988 and until 2014 June. After that, the source exhibited several ...
  • Ji L.; Ducci L.; Santangelo A.; Zhang S.; Suleimanov V.; Tsygankov S.; Doroshenko V.; Nabizadeh A.; Zhang S.N.; Ge M.Y.; Tao L.; Bu Q.C.; Qu J.L.; Lu F.J.; Chen L.; Song L.M.; Li T.P.; Xu Y.P.; Cao X.L.; Chen Y.; Liu C.Z.; Cai C.; Chang Z.; Chen G.; Chen T.X.; Chen Y.B.; Chen Y.P.; Cui W.; Cui W.W.; Deng J.K.; Dong Y.W.; Du Y.Y.; Fu M.X.; Gao G.H.; Gao H.; Gao M.; Gu Y.D.; Guan J.; Guo C.C.; Han D.W.; Huang Y.; Huo J.; Jia S.M.; Jiang L.H.; Jiang W.C.; Jin J.; Jin Y.J.; Kong L.D.; Li B.; Li C.K.; Li G.; Li M.S.; Li W.; Li X.; Li X.B.; Li X.F.; Li Y.G.; Li Z.W.; Liang X.H.; Liao J.Y.; Liu B.S.; Liu G.Q.; Liu H.X.; Liu H.W.; Liu X.J.; Liu Y.N.; Lu B.; Lu X.F.; Luo Q.; Luo T.; Ma X.; Meng B.; Nang Y.; Nie J.Y.; Ou G.; Sai N.; Shang R.C.; Song X.Y.; Sun L.; Tan Y.; Tuo Y.L.; Wang C.; Wang G.F.; Wang J.; Wang P.J.; Wang W.S.; Wang Y.S.; Wen X.Y.; Wu B.Y.; Wu B.B.; Wu M.; Xiao G.C.; Xiao S.; Xiong S.L.; Xu H.; Yang J.W.; Yang S.; Yang Y.J.; Yi Q.B. (2021)
    We report on our analysis of the 2019 outburst of the X-ray accreting pulsar 4U 1901+03 observed with Insight-HXMT and NICER. Both spectra and pulse profiles evolve significantly in the decaying phase of the outburst. ...
  • Punsly B.; Rodriguez J.; Trushkin S. (2016)
    © 2016. The American Astronomical Society. All rights reserved.The microquasar GRS 1915+105 is known for its spectacular discrete ejections. They occur unexpectedly, thus their inception has escaped direct observation. It ...
  • Koljonen K.; Maccarone T.; McCollough M.; Gurwell M.; Trushkin S.; Pooley G.; Piano G.; Tavani M. (2018)
    © ESO 2018. Context. Cygnus X-3 is a unique microquasar in the Galaxy hosting a Wolf-Rayet companion orbiting a compact object that most likely is a low-mass black hole. The unique source properties are likely due to the ...
  • Неизвестный автор (2018)
    © 2016 The Authors. We investigate whether the intrinsic spin of neutron stars (NSs) leaves an observable imprint on the spectral properties of X-ray binaries. To evaluate this, we consider a sample of nine NSs for which ...
  • Keek L.; Cumming A.; Wolf Z.; Ballantyne D.; Suleimanov V.; Kuulkers E.; Strohmayer T. (2015)
    © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Superbursts are hours-long X-ray flares attributed to the thermonuclear runaway burning of carbon-rich material in the ...
  • Kajava J.; Nättilä J.; Latvala O.; Pursiainen M.; Poutanen J.; Suleimanov V.; Revnivtsev M.; Kuulkers E.; Galloway D. (2014)
    © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. Neutron star (NS)masses and radii can be estimated from observations of photospheric radiusexpansion X-ray bursts, provided ...
  • Bozzo E.; Oskinova L.; Lobel A.; Hamann W. (2017)
    © ESO, 2017. The long-term X-ray light curves of classical supergiant X-ray binaries and supergiant fast X-ray transients show relatively similar super-orbital modulations, which are still lacking a sound interpretation. ...
  • Fabrika S.N.; Atapin K.E.; Vinokurov A.S.; Sholukhova O.N. (2021)
    Ultraluminous X-ray sources (ULXs) were identified as a separate class of objects in 2000 based on data from the Chandra X-Ray Observatory. These are unique objects: their X-ray luminosities exceed the Eddington limit for ...
  • Doroshenko V.; Santangelo A.; Suleimanov V. (2011)
    We present an analysis of the Vela X-1 "off-states" based on Suzaku observations taken in June 2008. Defined as states in which the flux suddenly decreases below the instrumental sensitivity, these "off-states" have been ...
  • Sokolova-Lapa E.; Gornostaev M.; Wilms J.; Ballhausen R.; Falkner S.; Postnov K.; Thalhammer P.; Fürst F.; García J.A.; Shakura N.; Becker P.A.; Wolff M.T.; Pottschmidt K.; Härer L.; Malacaria C. (2021)
    Recent observations of X-ray pulsars at low luminosities allow, for the first time, the comparison of theoretical models of the emission from highly magnetized neutron star atmospheres at low mass-accretion rates (M ≤ 1015 ...
  • Galiullin I.I.; Gilfanov M.R. (2021)
    Abstract: The X-ray emission from the counterparts of historical classical novae (CNe) in our Galaxy is studied. For this purpose, we use data from three SRG/eROSITA sky surveys in the half of the sky for the processing ...
  • Ji L.; Doroshenko V.; Suleimanov V.; Santangelo A.; Orlandini M.; Liu J.; Ducci L.; Zhang S.N.; Nabizadeh A.; Gavran D.; Zhang S.; Ge M.Y.; Li X.B.; Tao L.; Bu Q.C.; Qu J.L.; Lu F.J.; Chen L.; Song L.M.; Li T.P.; Xu Y.P.; Cao X.L.; Chen Y.; Liu C.Z.; Cai C.; Chang Z.; Chen T.X.; Chen Y.P.; Cui W.W.; Du Y.Y.; Gao G.H.; Gao H.; Gu Y.D.; Guan J.; Guo C.C.; Han D.W.; Huang Y.; Huo J.; Jia S.M.; Jiang W.C.; Jin J.; Kong L.D.; Li B.; Li C.K.; Li G.; Li W.; Li X.; Li X.F.; Li Z.W.; Liang X.H.; Liao J.Y.; Liu B.S.; Liu H.X.; Liu H.W.; Liu X.J.; Lu X.F.; Luo Q.; Luo T.; Ma R.C.; Ma X.; Meng B.; Nang Y.; Nie J.Y.; Ou G.; Ren X.Q.; Sai N.; Song X.Y.; Sun L.; Tan Y.; Tuo Y.L.; Wang C.; Wang L.J.; Wang P.J.; Wang W.S.; Wang Y.S.; Wen X.Y.; Wu B.Y.; Wu B.B.; Wu M.; Xiao G.C.; Xiao S.; Xiong S.L.; Yang R.J.; Yang S.; Yang Y.J.; Yi Q.B.; Yin Q.Q.; You Y.; Zhang F.; Zhang H.M.; Zhang J.; Zhang P.; Zhang W.; Zhang W.C.; Zhang Y.; Zhang Y.F.; Zhang Y.H.; Zhao H.S.; Zhao X.F. (2021)
    We investigate the absorption and emission features in observations of GX 301-2 detected with Insight-HXMT/LE in 2017-2019. At different orbital phases, we found prominent Fe Kα, Kβ, and Ni Kα lines, as well as Compton ...
  • Atapin K.; Fabrika S.; Medvedev A.; Vinokurov A. (2015)
    © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. We study a stochastic variability of SS 433 in the 10-4-5 × 10-2 Hz frequency range based on RXTE data, and on simultaneous ...
  • Sanjurjo-Ferrín G.; Torrejón J.M.; Postnov K.; Oskinova L.; Rodes-Roca J.J.; Bernabeu G. (2021)
    Cen X-3 is a compact high-mass X-ray binary likely powered by Roche lobe overflow. We present a phase-resolved X-ray spectral and timing analysis of two pointed XMM-Newton observations. The first one took place during a ...

Поиск в электронном архиве


Расширенный поиск

Просмотр

Моя учетная запись