activity
20232026
most citedSIROCCO: A Publicly Available Monte Carlo Ionization and Radiative Transfer Code for Astrophysical Outflows

14 citations · 28 across the 17 of their papers we have counts for

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Showing 2025Show all

7 papers · 1 filter

astro-ph.GA2025

The critical role of clumping in line-driven disc winds

Amin Mosallanezhad, Christian Knigge, Nicolas Scepi +4

Radiation pressure on spectral lines is a promising mechanism for powering disc winds from accreting white dwarfs (AWDs) and active galactic nuclei (AGN). However, in radiation-hyd…

astro-ph.HE2025★ 1 cited

Further evidence for natal kick segregation by spectral type in high-mass X-ray binaries

Pornisara Nuchvanichakul, Poshak Gandhi, Christian Knigge +4

High-mass X-ray binaries (HMXBs) are systems in which a neutron star or black hole accretes material from a massive companion. HMXBs are expected to have experienced a supernova in…

astro-ph.IM2025★ 1 cited

A Diagnostic Kit for Optical Emission Lines Shaped by Accretion Disc Winds

Austen G. W. Wallis, Christian Knigge, James H. Matthews +2

Blueshifted absorption is the classic spectroscopic signature of an accretion disc wind in X-ray binaries and cataclysmic variables (CVs). However, outflows can also create pure em…

astro-ph.HE2025

Evolution of the inner accretion flow and the white-dwarf spin pulse during the 2023 outburst in GK Persei

Mariko Kimura, Takayuki Hayashi, Yuuki Wada +8

We present our X-ray and optical observations performed by NICER, NuSTAR, and Tomo-e Gozen during the 2023 outburst in the intermediate polar GK Persei. The X-ray spectrum consiste…

astro-ph.HE2025★ 1 cited

On the distance to the black hole X-ray binary Swift J1727.81613

Benjamin J. Burridge, James C. A. Miller-Jones, Arash Bahramian +11

We review the existing distance estimates to the black hole X-ray binary Swift J1727.81613, present new radio and near-UV spectra to update the distance constraints, and discuss…

astro-ph.HE2025★ 1 cited

Ultraviolet spectroscopy of the black hole X-ray binary MAXI J1820+070 across a state transition

Maria Georganti, Christian Knigge, Noel Castro Segura +8

We present ultraviolet (UV) spectroscopic observations covering three distinct accretion states of the low-mass X-ray binary (LMXB) MAXI J1820+070: the luminous hard state, a hard-…

astro-ph.SR2025

Characterisation of H spectra from EXO 051910+3737.7 X-rays binaries

Pornisara Nuchvanichakul, Puji Irawati, Pakakaew Rittipruk +4

We investigate the spectral characteristics of the Be/X-ray binary system, EXO 051910+3737.7, in which Be/X-ray systems are the largest sub-class of high-mass X-ray binaries. Spect…