activity
20092026
most citedThe eROSITA X-ray telescope on SRG

884 citations · 7.7k across the 224 of their papers we have counts for

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Showing 2017Show all

5 papers · 1 filter

astro-ph.HE2017★ 69 cited

Orbit and intrinsic spin-up of the newly discovered transient X-ray pulsar Swift J0243.6+6124

Victor Doroshenko, Sergey Tsygankov, Andrea Santangelo

We present the orbital solution for the newly discovered transient Be X-ray binary Swift J0243.6+6124 based on the data from gamma-ray burst monitor onboard Fermi obtained during t…

astro-ph.HE2017★ 17 cited

XMM-Newton observations of the non-thermal supernova remnant HESS J1731-347 (G353.6-0.7)

V. Doroshenko, G. Pühlhofer, A. Bamba +4

We report on the analysis of XMM-Newton observations of the non-thermal shell-type supernova remnant HESS J1731-347 (G353.6-0.7). For the first time the complete remnant shell has…

astro-ph.HE2017★ 71 cited

Stable accretion from a cold disc in highly magnetized neutron stars

S. S. Tsygankov, A. A. Mushtukov, V. F. Suleimanov +4

The aim of this paper is to investigate the transition of a strongly magnetized neutron star into the accretion regime with very low accretion rate. For this purpose we monitored t…

astro-ph.HE2017★ 13 cited

BeppoSAX observations of XTE J1946+274

R. Doroshenko, A. Santangelo, V. Doroshenko +1

We report on the BeppoSAX monitoring of a giant outburst of the transient X-ray pulsar XTE J1946+274 in 1998. The source was detected with a flux of ~ 4 x 10^(-9) erg cm^(-2) s^(-1…

astro-ph.HE2017★ 104 cited

SMC X-3: the closest ultraluminous X-ray source powered by a neutron star with non-dipole magnetic field

S. S. Tsygankov, V. Doroshenko, A. A. Lutovinov +2

Magnetic field of accreting neutron stars determines their overall behaviour including the maximum possible luminosity. Some models require an above-average magnetic field strength…