activity
20132026
most citedAlternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1

142 citations · 2.2k across the 57 of their papers we have counts for

collaborators

57 papers

astro-ph.HE2026

Early results from the SVOM Observatory Science program

A. Coleiro, L. Tao, F. Cangemi +44

We present the organisation and early results from the Observatory Science program of the Space-based multi-band astronomical Variable Objects Monitor (SVOM), based on data collect…

astro-ph.HE2024

X-ray measurement of a high-mass white dwarf and its spin for the intermediate polar IGR J18434-0508

Julian Gerber, Jeremy Hare, John A. Tomsick +8

IGR J18434-0508 is a Galactic Intermediate Polar (IP) type Cataclysmic Variable (CV) previously classified through optical spectroscopy. The source is already known to have a hard…

astro-ph.HE2024★ 12 cited

Impact of the disk magnetization on MHD disk wind signature

Sudeb Ranjan Datta, Susmita Chakravorty, Jonathan Ferreira +8

Observation of blue-shifted X-ray absorption lines indicates the presence of wind from the accretion disk in X-ray binaries. Magnetohydrodynamic (MHD) driving is one of the possibl…

astro-ph.HE2023★ 8 cited

Classifying IGR J15038-6021 as a magnetic CV with a massive white dwarf

John A. Tomsick, Snehaa Ganesh Kumar, Benjamin M. Coughenour +8

Cataclysmic variables (CVs) are binary systems consisting of a white dwarf (WD) accreting matter from a companion star. Observations of CVs provide an opportunity to learn about ac…

astro-ph.HE2022★ 15 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.HE2022★ 23 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…