Rapid X-ray variability
M Van der Klis - Cambridge Astrophysics Series, 2006 - cambridge.org
One of the principal motivations for studying X-ray binaries is that accretion onto neutron
stars and black holes provides a unique window on the physics of strong gravity and dense …
stars and black holes provides a unique window on the physics of strong gravity and dense …
Global optical/infrared–X-ray correlations in X-ray binaries: quantifying disc and jet contributions
DM Russell, RP Fender, RI Hynes… - Monthly Notices of …, 2006 - academic.oup.com
The optical/near-infrared (OIR) region of the spectra of low-mass X-ray binaries (XBs)
appears to lie at the intersection of a variety of different emission processes. In this paper we …
appears to lie at the intersection of a variety of different emission processes. In this paper we …
Parameters of the X-ray binary system Scorpius X-1
AM Cherepashchuk, TS Khruzina… - Monthly Notices of the …, 2021 - academic.oup.com
We modelled optical light curves of Sco X-1 obtained by the Kepler Space Telescope during
the K 2 mission. Modelling was performed for the case of strong heating of the optical star …
the K 2 mission. Modelling was performed for the case of strong heating of the optical star …
[PDF][PDF] A review of rapid X-ray variability in X-ray binaries
M van der Klis - arXiv preprint astro-ph/0410551, 2004 - arxiv.org
arXiv:astro-ph/0410551v1 22 Oct 2004 Page 1 arXiv:astro-ph/0410551v1 22 Oct 2004 Contents
2 Rapid X-Ray Variability page 1 2.1 Introduction 1 2.2 Timing 3 2.3 Spectroscopy 5 2.4 …
2 Rapid X-Ray Variability page 1 2.1 Introduction 1 2.2 Timing 3 2.3 Spectroscopy 5 2.4 …
Parameters of X-Ray Binary Sco X-1 in the Model of Partial Filling of Roche Lobe by Optical Star
AM Cherepashchuk, TS Khruzina, AI Bogomazov - Astronomy Reports, 2022 - Springer
We have simulated optical orbital light curves of the Sco X-1 system obtained by the Kepler
space observatory during K2 mission. Simulation was carried out under assumption that the …
space observatory during K2 mission. Simulation was carried out under assumption that the …
Polarized infrared emission from X-ray binary jets
DM Russell, RP Fender - Monthly Notices of the Royal …, 2008 - academic.oup.com
Near-infrared (NIR) and optical polarimetric observations of a selection of X-ray binaries are
presented. The targets were observed using the Very Large Telescope and the United …
presented. The targets were observed using the Very Large Telescope and the United …
A hard X-ray view of Scorpius X-1 with INTEGRAL: Nonthermal emission?
T Di Salvo, P Goldoni, L Stella… - The Astrophysical …, 2006 - iopscience.iop.org
We present here simultaneous INTEGRAL/RXTE observations of Sco X-1 and in particular a
study of the hard X-ray emission of the source and its correlation with the position in the Z …
study of the hard X-ray emission of the source and its correlation with the position in the Z …
Links between optical and X-ray light in Scorpius X-1
AB Igl, RI Hynes, CT Britt, KS O'Brien… - Monthly Notices of the …, 2023 - academic.oup.com
We observed the low-mass X-ray binary Sco X-1 for 12 nights simultaneously using the
Rossi X-Ray Timing Explorer and the Otto Struve Telescope at McDonald Observatory at 1-s …
Rossi X-Ray Timing Explorer and the Otto Struve Telescope at McDonald Observatory at 1-s …
Kepler K2 observations of Sco X-1: orbital modulations and correlations with Fermi GBM and MAXI
RI Hynes, BE Schaefer, ZA Baum… - Monthly Notices of …, 2016 - academic.oup.com
We present a multi-wavelength study of the low-mass X-ray binary Sco X-1 using Kepler K2
optical data and Fermi GBM and MAXI X-ray data. We recover a clear sinusoidal orbital …
optical data and Fermi GBM and MAXI X-ray data. We recover a clear sinusoidal orbital …
Period–luminosity relation for persistent low‐mass X‐ray binaries in the near‐infrared
MG Revnivtsev, IY Zolotukhin… - Monthly Notices of the …, 2012 - academic.oup.com
We study the relations between the X‐ray luminosity, orbital period and absolute near‐
infrared magnitude of persistent low‐mass X‐ray binaries (LMXBs). We show that often the …
infrared magnitude of persistent low‐mass X‐ray binaries (LMXBs). We show that often the …