[HTML][HTML] Ultraluminous X-ray sources
The study of ultraluminous X-ray sources (ULXs) has changed dramatically over the last
decade. In this review we first describe the most important observations of ULXs in various …
decade. In this review we first describe the most important observations of ULXs in various …
[HTML][HTML] Advances in understanding high-mass X-ray binaries with INTEGRALand future directions
High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as
in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology …
in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology …
Cyclotron lines in highly magnetized neutron stars
R Staubert, J Trümper, E Kendziorra… - Astronomy & …, 2019 - aanda.org
Cyclotron lines, also called cyclotron resonant scattering features are spectral features,
generally appearing in absorption, in the X-ray spectra of objects containing highly …
generally appearing in absorption, in the X-ray spectra of objects containing highly …
Optically thick envelopes around ULXs powered by accreating neutron stars
AA Mushtukov, VF Suleimanov… - Monthly Notices of …, 2017 - academic.oup.com
Magnetized neutron stars power at least some ultraluminous X-ray sources. The accretion
flow in these cases is interrupted at the magnetospheric radius and then reaches the surface …
flow in these cases is interrupted at the magnetospheric radius and then reaches the surface …
The gas-to-extinction ratio and the gas distribution in the Galaxy
H Zhu, W Tian, A Li, M Zhang - Monthly Notices of the Royal …, 2017 - academic.oup.com
We investigate the relation between the optical extinction (AV) and the hydrogen column
density (NH) determined from X-ray observations of a large sample of Galactic sightlines …
density (NH) determined from X-ray observations of a large sample of Galactic sightlines …
Accreting Neutron Stars in 3D General-relativistic Magnetohydrodynamic Simulations: Jets, Magnetic Polarity, and the Interchange Slingshot
Accreting neutron stars differ from black holes by the presence of the star's own magnetic
field, whose interaction with the accretion flow is a central component in understanding …
field, whose interaction with the accretion flow is a central component in understanding …
SMC X-3: the closest ultraluminous X-ray source powered by a neutron star with non-dipole magnetic field
Aims. The magnetic field of accreting neutron stars determines their overall behavior
including the maximum possible luminosity. Some models require an above-average …
including the maximum possible luminosity. Some models require an above-average …
Luminosity dependence of the cyclotron line and evidence for the accretion regime transition in V 0332+ 53
We report on the analysis of NuSTAR observations of the Be-transient X-ray pulsar V 0332+
53 during the giant outburst in 2015 and another minor outburst in 2016. We confirm the …
53 during the giant outburst in 2015 and another minor outburst in 2016. We confirm the …
The 2019 super-Eddington outburst of RX J0209. 6− 7427: detection of pulsations and constraints on the magnetic field strength
G Vasilopoulos, PS Ray, KC Gendreau… - Monthly Notices of …, 2020 - academic.oup.com
In 2019 November, MAXI detected an X-ray outburst from the known Be X-ray binary system
RX J0209. 6− 7427 located in the outer wing of the Small Magellanic Cloud. We followed the …
RX J0209. 6− 7427 located in the outer wing of the Small Magellanic Cloud. We followed the …
An evolving jet from a strongly magnetized accreting X-ray pulsar
Relativistic jets are observed throughout the Universe and strongly affect their surrounding
environments on a range of physical scales, from Galactic binary systems to galaxies and …
environments on a range of physical scales, from Galactic binary systems to galaxies and …