Results 121 to 130 of about 5,289 (173)

Energy Flow and Radiation Efficiency in Radiative GRMHD Simulations of Neutron Star Ultraluminous X-Ray Sources

open access: yesThe Astrophysical Journal
We investigate numerically the energy flow and radiation efficiency of accreting neutron stars as potential ultraluminous X-ray sources (ULXs). We perform 10 simulations in radiative general relativistic magnetohydrodynamics, exploring six different ...
Fatemeh Kayanikhoo   +3 more
doaj   +1 more source

Multiwavelength Observations of the Apparently Nonrepeating FRB 20250316A

open access: yesThe Astrophysical Journal
The physical origin of fast radio bursts (FRBs) remains uncertain. Although multiwavelength observations have been widely conducted, only Galactic FRB 20200428D is associated with an X-ray burst from the magnetar SGR J1935+2154.
Ye Li   +74 more
doaj   +1 more source

Spectral Calculations of 3D Radiation Magnetohydrodynamic Simulations of Super-Eddington Accretion onto a Stellar-mass Black Hole

open access: yesThe Astrophysical Journal
We use the Athena++ Monte Carlo (MC) radiation transfer module to postprocess simulation snapshots from nonrelativistic Athena++ radiation magnetohydrodynamic (RMHD) simulations. These simulations were run using a gray (frequency-integrated) approach but
Brianna S. Mills   +3 more
doaj   +1 more source

From Feast to Famine: A Systematic Study of Accretion onto Oblique Pulsars with 3D GRMHD Simulations

open access: yesThe Astrophysical Journal Letters
Disk-fed accretion onto neutron stars can power a wide range of astrophysical sources ranging from X-ray binaries, to accretion-powered millisecond pulsars, ultraluminous X-ray sources, and gamma-ray bursts.
Ariadna Murguia-Berthier   +3 more
doaj   +1 more source

Theoretical Analysis of the RX J0209.6−7427 X-Ray Spectrum during a Giant Outburst

open access: yesThe Astrophysical Journal Letters
We model the spectral formation occurring in the binary X-ray pulsar (XRP) RX J0209.6−7427 during the 2019 super-Eddington outburst. Using a theoretical model previously developed by the authors, we are able to produce spectra that closely resemble the ...
Brent F. West   +2 more
doaj   +1 more source

Colliding winds in ultraluminous X-ray sources

open access: yes, 2022
Fil: Abaroa, Leandro. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas.
Abaroa, Leandro   +2 more
openaire   +3 more sources

A Striking Confluence Between Theory and Observations of High-Mass X-ray Binary Pulsars. [PDF]

open access: yesRes Astron Astrophys, 2018
Christodoulou DM   +2 more
europepmc   +1 more source

The Great Pretenders Among the ULX Class. [PDF]

open access: yesRes Astron Astrophys, 2017
Christodoulou DM   +4 more
europepmc   +1 more source

Detection of the Optical Counterpart of the Transient ULX NGC 300 ULX-1: A Nascent Black Hole-neutron Star Binary?

open access: yesThe Astrophysical Journal
The endpoints of massive star evolution are poorly known, especially those in interacting binary systems containing compact objects, such as neutron stars or black holes (BHs).
André-Nicolas Chené   +3 more
doaj   +1 more source

<i>NICER</i> and <i>Fermi</i> GBM Observations of the First Galactic Ultraluminous X-ray Pulsar Swift J0243.6+6124. [PDF]

open access: yesAstrophys J, 2018
Wilson-Hodge CA   +21 more
europepmc   +1 more source

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