papers

Publications (25)

astro-ph.HE2022

Orbital decay in M82 X-2

Matteo Bachetti, Marianne Heida, Thomas Maccarone +21

M82 X-2 is the first pulsating ultraluminous X-ray source (PULX) discovered. The luminosity of these extreme pulsars, if isotropic, implies an extreme mass transfer rate. An altern…

astro-ph.HE2021

Long-term X-ray spectral evolution of Ultraluminous X-ray sources: implications on the accretion flow geometry and the nature of the accretor

Andrés Gúrpide, Olivier Godet, Filippos Koliopanos +2

The discovery of pulsations in several Ultraluminous X-ray sources (ULXs) demonstrated that a fraction of ULXs are powered by super-Eddington accretion onto neutron stars (NSs). Th…

astro-ph.HE2021

Probabilistic classification of X-ray sources applied to Swift-XRT and XMM-Newton catalogs

Hugo Tranin, Olivier Godet, Natalie Webb +1

Context. Serendipitous X-ray surveys have proven to be an efficient way to find rare objects, for example tidal disruption events, changing-look active galactic nuclei (AGN), binar…

astro-ph.HE2020

Disappearance of the Fe K emission line in Ultra Compact X-ray Binaries 4U 1543-624 and Swift J1756.9-2508

Filippos Koliopanos, Georgios Vasilopoulos, Sebastien Guillot +1

We investigate the long-term variability of the K line of iron in the spectra of two Ultra Compact X-ray Sources (UCXBs) with C/O-rich donors. We revisit archival observations…

astro-ph.HE2013

The Hot and Energetic Universe: End points of stellar evolution

Christian Motch, Jörn Wilms, Didier Barret +22

White dwarfs, neutron stars and stellar mass black holes are key laboratories to study matter in most extreme conditions of gravity and magnetic field. The unprecedented effective…

astro-ph.HE2013

Radio Detections During Two State Transitions of the Intermediate Mass Black Hole HLX-1

Natalie Webb, David Cseh, Emil Lenc +7

Relativistic jets are streams of plasma moving at appreciable fractions of the speed of light. They have been observed from stellar mass black holes (320 solar masses, M$_…