87 citations · 319 across the 10 of their papers we have counts for
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Long-term pulse profile study of the Be/X-ray pulsar SAX J2103.5+4545
A. Camero Arranz, C. A. Wilson, M. H. Finger +1
Aims. We present the first long-term pulse profile study of the X-ray pulsar SAX J2103.5+4545. Our main goal is to study the pulse shape correlation either with luminosity, time or…
A 0535+26 in the August/September 2005 outburst observed by RXTE and INTEGRAL
I. Caballero, P. Kretschmar, A. Santangelo +14
In this Letter we present results from INTEGRAL and RXTE observations of the spectral and timing behavior of the High Mass X-ray Binary A 0535+26 during its August/September 2005 n…
A Possible Magnetar Nature for IGR J16358-4726
S. K. Patel, J. Zurita, M. Del Santo +10
We present detailed spectral and timing analysis of the hard x-ray transient IGR J16358-4726 using multi-satellite archival observations. A study of the source flux time history ov…
INTEGRAL observations of the Be/X-ray binary EXO 2030+375 during outburst
A. Camero Arranz, C. A. Wilson, P. Connell +4
We present a type-I outburst of the high-mass X-ray binary EXO 2030+375, detected during INTEGRAL's Performance and Verification Phase in December 2002 (on-source time about 10e+06…
XTE J0111.2-7317 : a nebula-embedded X-ray binary in the SMC
M. J. Coe, N. J. Haigh, C. A. Wilson +1
The observed characteristics of the nebulosity surrounding the SMC High Mass X-ray Binary XTE J0111.2-7317 are examined in the context of three possible nebular types: SNR, bowshoc…
Long-term Properties of Accretion Disks in X-ray Binaries: I. the variable third period in SMC X-1
W. I. Clarkson, P. A. Charles, M. J. Coe +3
Long term X-ray monitoring data from the RXTE ASM and CGRO BATSE reveal that the third (superorbital) period in SMC X-1 is not constant, but varies between 40-60 days. A dynamic po…