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Orbital parameters of V 0332+53 from 2015 giant outburst data
V. Doroshenko, S. Tsygankov, A. Santangelo
We present the updated orbital solution for the transient Be X-ray binary V 0332+53 comple- menting historical measurements with the data from the gamma-ray burst monitor onboard F…
Evidence for a binary origin of a central compact object
Victor Doroshenko, Gerd Puehlhofer, Patrick Kavanagh +3
Central compact objects (CCOs) are thought to be young thermally emitting isolated neutron stars that were born during the preceding core-collapse supernova explosion. Here we pres…
Properties and observability of glitches and anti-glitches in accreting pulsars
L. Ducci, P. M. Pizzochero, V. Doroshenko +3
Several glitches have been observed in young, isolated radio pulsars, while a clear detection in accretion-powered X-ray pulsars is still lacking. We use the Pizzochero snowplow mo…
BeppoSAX observations of GRO J1744-28
R. Doroshenko, A. Santangelo, V. Doroshenko +2
We present an analysis of BeppoSAX observations of the unique transient bursting X-ray pulsar GRO J1744-28. The observations took place in March 1997 during the decay phase of the…
Transient X-ray pulsar V0332+53: pulse phase-resolved spectroscopy and the reflection model
A. A. Lutovinov, S. S. Tsygankov, V. F. Suleimanov +4
We present the results of the pulse phase- and luminosity-resolved spectroscopy of the transient X-ray pulsar V0332+53, performed for the first time in a wide luminosity range (1-4…
Probing stellar winds and accretion physics in high-mass X-ray binaries and ultra-luminous X-ray sources with LOFT
M. Orlandini, V. Doroshenko, L. Zampieri +28
This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT f…