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Просмотр по автору "Wilms J."

Просмотр по автору "Wilms J."

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  • Investigating the Mini and Giant Radio Flare Episodes of Cygnus X-3 
    Egron E.; Pellizzoni A.; Righini S.; Giroletti M.; Koljonen K.; Pottschmidt K.; Trushkin S.; Lobina J.; Pilia M.; Wilms J.; Corbel S.; Grinberg V.; Loru S.; Trois A.; Rodriguez J.; Lähteenmäki A.; Tornikoski M.; Enestam S.; Järvelä E. (2020)
    © 2020. The American Astronomical Society. All rights reserved. The microquasar Cygnus X-3 underwent a giant radio flare in 2017 April, reaching a maximum flux of ∼16.5 Jy at 8.5 GHz. We present results from a long monitoring ...
  • Modelling of 35-d superorbital cycle of B and V light curves of IMXB HZ Her/Her X-1 
    Kolesnikov D.A.; Shakura N.I.; Postnov K.A.; Volkov I.M.; Bikmaev I.F.; Irsmambetova T.R.; Staubert R.; Wilms J.; Irtuganov E.; Golysheva P.Y.; Shugarov S.Y.; Nikolenko I.V.; Trunkovsky E.M.; Schönherr G.; Schwope A.; Klochkov D. (2020)
    © 2020 The Author(s). The X-ray binary Her X-1 consists of an accreting neutron star and the optical component HZ Her. The 35-d X-ray superorbital variability of this system is known, since its discovery in 1972 by the ...
  • The 35-day cycle in the X-ray binary HZ Her/Her X-1 
    Kolesnikov D.; Shakura N.; Postnov K.; Volkov I.; Bikmaev I.; Irsmambetova T.; Staubert R.; Wilms J.; Irtuganov E.; Shurygin P.; Golysheva P.; Shugarov S.; Nikolenko I.; Trunkovsky E.; Schonherr G.; Schwope A.; Klochkov D. (2020)
    © 2020 Astronomical Institute, Slovak Academy of Sciences. We present the results of modelling the 35-day superorbital changes in the B and V lightcurves and X-ray flux of HZ Her/Her X-1. The model is implemented in a ...
  • The double-degenerate nucleus of the planetary nebula TS01: A close binary evolution showcase 
    Tovmassian G.; Yungelson L.; Rauch T.; Suleimanov V.; Napiwotzki R.; Stasińska G.; Tomsick J.; Wilms J.; Morisset C.; Pẽa M.; Richer M. (2010)
    We present a detailed investigation of SBS1150+599A, a close binary star hosted by the planetary nebula PNG135.9+55.9 (TS 01). The nebula, located in the Galactic halo, is the most oxygen-poor known to date and is the only ...
  • X-ray emission from magnetized neutron star atmospheres at low mass-accretion rates: I. Phase-averaged spectrum 
    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 ...

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