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Probing the behaviour of the X-ray binary Cygnus X-3 with very-long-baseline radio interferometry

(2009)

Authors:

V Tudose, JCA Miller-Jones, RP Fender, Z Paragi, C Sakari, A Szostek, MA Garrett, V Dhawan, A Rushton, RE Spencer, M van der Klis
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'Disc-jet' coupling in black hole X-ray binaries and active galactic nuclei

(2009)
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Following the 2008 outburst decay of the black hole candidate H1743-322 in X-ray and radio

(2009)

Authors:

PG Jonker, J Miller-Jones, J Homan, E Gallo, M Rupen, J Tomsick, RP Fender, P Kaaret, DTH Steeghs, MAP Torres, R Wijnands, S Markoff, WHG Lewin
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The proper motion and changing jet morphology of Cygnus X-3

(2009)

Authors:

JCA Miller-Jones, CM Sakari, V Dhawan, V Tudose, RP Fender, Z Paragi, MA Garrett
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Refined orbital solution and quiescent variability in the black hole transient GS 1354-64 (= BW Cir)

Astrophysical Journal, Supplement Series 181:1 (2009) 238-243

Authors:

J Casares, JA Orosz, C Zurita, T Shahbaz, JM Corral-Santana, JE Mcclintock, MR Garcia, IG Martínez-Pais, PA Charles, RP Fender, RA Remillard

Abstract:

In Casares et al. we presented the first radial velocity curve of the companion star to BW Cir which demonstrates the presence of a black hole in this historical X-ray transient. But these data were affected by aliasing and two possible periods at 2.5445 days and 2.5635 days were equally possible. Here we present new spectroscopic data that enable us to break the 1-year aliasing and confirm 2.5445 days as the correct orbital period. We also present R-band photometry over 14 years, which reveals the presence of important flaring activity dominating the light curves. © 2009. The American Astronomical Society. All rights reserved.
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