activity
20182026
most citedNuSTAR/XMM-Newton monitoring of the Seyfert 1 galaxy HE 1143-1810. Testing the two-corona scenario

52 citations · 237 across the 9 of their papers we have counts for

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14 papers · 1 filter

astro-ph.HE2026

Spectro-polarimetric study of the black hole X-ray binary Swift J1727.8-1613 in the JED-SAD framework

R. Muhammad, P. -O. Petrucci, W. Zhang +10

Context. Swift J1727.8-1613 is an X-ray binary observed during its 2023-2024 outburst, including bright and dim hard states with similar X-ray polarimetric signatures but fluxes di…

astro-ph.HE20249 cited

Thermal solutions of strongly magnetized disks and the hysteresis in X-ray binaries

Nicolas Scepi, Jason Dexter, Mitchell C. Begelman +3

X-ray binaries (XRBs) exhibit spectral hysteresis for luminosities in the range , with a hard X-ray spectral state that persists from…

astro-ph.HE20231 cited

The jet emitting disk standard accretion disk model applied to the active galactic nuclei ultra violet Xray correlation

Samuel Barnier, Pierre-Olivier Petrucci, Jonathan Ferreira +1

The non linear correlation between the UV and X-ray emission observed in Active Galactic Nuclei remains a puzzling question that challenged accretion models. While the UV emission…

astro-ph.HE202215 cited

Absorption lines from magnetically driven winds in X-ray binaries II: high resolution observational signatures expected from future X-ray observatories

Susmita Chakravorty, Pierre-Olivier Petrucci, Sudeb Ranjan Datta +12

In our self-similar, analytical, magneto-hydrodynamic (MHD) accretion-ejection solution, the density at the base of the outflow is explicitly dependent on the disk accretion rate -…

astro-ph.HE202223 cited

Are Low-Frequency Quasi-Periodic Oscillations seen in accretion flows the disk response to a jet instability?

Jonathan Ferreira, Gregoire Marcel, Pierre-Olivier Petrucci +7

Low Frequency Quasi-Periodic Oscillations or LF QPOs are ubiquitous in BH X-ray binaries and provide strong constraints on the accretion-ejection processes. Although several models…

astro-ph.HE2021

Expected disk wind properties evolution along an X-ray Binary outburst

P. -O. Petrucci, S. Bianchi, G. Ponti +12

Blueshifted X-ray absorption lines (preferentially from Fe XXV and Fe XXVI present in the 6-8 keV range) indicating the presence of massive hot disk winds in Black Hole (BH) X-ray…