Results 81 to 90 of about 195 (150)
On the physical nature of the source of ultraluminous X-ray pulsations [PDF]
Extended and revised version, which will appear in Astrophysics and Space Science (ASTR-D-15-00411R2-accepted).
openaire +2 more sources
Possible Supercritical Accretion on the Ultraluminous X-Ray Source in the Metal-poor Galaxy I Zw 18
We present an analysis of X-ray observations of the ultraluminous X-ray source (ULX) in I Zw 18 based on archival data taken with Chandra, XMM-Newton, and Suzaku. This ULX is considered to be an intermediate-mass black hole candidate simply because it is
Marina Yoshimoto +4 more
doaj +1 more source
Extensive astronomical surveys, like those conducted with the Chandra X-ray Observatory, detect hundreds of thousands of unidentified cosmic sources. Machine learning (ML) methods offer an efficient, probabilistic approach to classifying them, which can ...
Shivam Kumaran +2 more
doaj +1 more source
Isomer-specific kinetics of the C+ + H2O reaction at the temperature of interstellar clouds. [PDF]
Yang T +7 more
europepmc +1 more source
Synchrotron Radiation from NGC 470 HLX1—a Hidden Hyperluminous Accreting Neutron Star?
We present the first broadband spectral analysis of NGC 470 HLX1, a hyperluminous X-ray source (HLX) that exhibits significant flux variability over different epochs.
Tanuman Ghosh +5 more
doaj +1 more source
An Alternative Model for the Orbital Decay of M82 X-2: The Anomalous Magnetic Braking of a Bp Star
Recently, the first pulsating ultraluminous X-ray source M82 X-2 was reported to be experiencing a rapid orbital decay at a rate of $\dot{P}=-(5.69\pm 0.24)\times {10}^{-8}\,{\rm{s}}\,{{\rm{s}}}^{-1}$ based on 7 yr NuSTAR data.
Wen-Cong Chen
doaj +1 more source
Electromagnetic counterparts to massive black-hole mergers. [PDF]
Bogdanović T, Miller MC, Blecha L.
europepmc +1 more source
A Deeper Look into eFEDS AGN Candidates in Dwarf Galaxies with Chandra
The ability to accurately discern active massive black holes (BHs) in nearby dwarf galaxies is paramount to understanding the origins and processes of “seed” BHs in the early Universe.
Adonis A. Sanchez +3 more
doaj +1 more source
Search for Fast Radio Bursts and Radio Pulsars from Pulsing Ultraluminous X-Ray Sources
We conducted targeted fast radio burst (FRB) and pulsar searches on eight pulsing ultraluminous X-ray sources (PULXs) using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) and the Parkes 64 m Radio Telescope (Murriyang) to investigate ...
Juntao Bai +7 more
doaj +1 more source
Modeling Reflection Spectra of Super-Eddington X-Ray Sources
Relativistic reflection is a common feature in the X-ray observations of accreting compact objects. We present reflux , a new X-ray reflection model for spectral analysis of super-Eddington sources.
Swarnim Shashank +7 more
doaj +1 more source

