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19982007
most citedOrbital X-Ray Variability of the Microquasar LS 5039

86 citations · 125 across the 4 of their papers we have counts for

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7 papers · 1 filter

astro-ph20075 cited

Supergiant Fast X-ray Transients: A common behaviour or a class of objects?

Ignacio Negueruela, David M. Smith, Jose Miguel Torrejon +1

INTEGRAL monitoring of the Galactic Plane is revealing a growing number of recurrent X-ray transients, characterised by short outbursts with very fast rise times (~ tens of minutes…

astro-ph2007

A jet model for black-hole X-ray sources

N. D. Kylafis, I. E. Papadakis, P. Reig

A jet model for Galactic black-hole X-ray binaries will be presented that appears to explain several observational characteristics. In particular, it explains the energy spectrum f…

astro-ph200586 cited

Orbital X-Ray Variability of the Microquasar LS 5039

V. Bosch-Ramon, J. M. Paredes, M. Ribo +3

The properties of the orbit and the donor star in the high mass X-ray binary microquasar LS 5039 indicate that accretion processes should mainly occur via a radiatively driven wind…

astro-ph200534 cited

Further evidence for the presence of a neutron star in 4U 2206+54. INTEGRAL and VLA observations

P. Blay, M. Ribo, I. Negueruela +5

The majority of High Mass X-ray Binaries (HMXBs) behave as X-ray pulsars, revealing that they contain a magnetised neutron star. Among the four HMXBs not showing pulsations, and th…

astro-ph1999

X-ray and radio observations of RX J1826.2-1450/LS 5039

M. Ribo, P. Reig, J. Marti +1

RX J1826.2-1450/LS 5039 has been recently proposed to be a radio emitting high mass X-ray binary. In this paper, we present an analysis of its X-ray timing and spectroscopic proper…

astro-ph1999

On the nature of the X-ray source 1E 1024.0--5732/Wack 2134

Pablo Reig

Two different models have been put forward to explain the origin of the X-ray emission of the unusual X-ray source 1E 1024.0-5732/Wack 2134: a high-mass X-ray binary system (HMXB)…