activity
20042009
most citedXMM-Newton and INTEGRAL spectroscopy of the microquasar GRO J1655-40 during its 2005 outburst

51 citations · 115 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.HE20095 cited

The Behavior of Matter under Extreme Conditions

F. Paerels, M. Mendez, M. Agueros +29

The cores of neutron stars harbor the highest matter densities known to occur in nature, up to several times the densities in atomic nuclei. Similarly, magnetic field strengths can…

astro-ph.HE20093 cited

Stellar-Mass Black Holes and Their Progenitors

J. M. Miller, P. Uttley, K. Nandra +14

If a black hole has a low spin value, it must double its mass to reach a high spin parameter. Although this is easily accomplished through mergers or accretion in the case of super…

astro-ph200821 cited

INTEGRAL and XMM-Newton Spectroscopy of GX 339-4 During Hard/Soft Intermediate and High/Soft States in the 2007 Outburst

M. D. Caballero-Garcia, J. M. Miller, M. Diaz Trigo +5

We present simultaneous XMM-Newton and INTEGRAL observations of the luminous black hole transient and relativistic jet source GX 339-4. GX 339-4 started an outburst on November of…

astro-ph200835 cited

Variations in the dip properties of the low-mass X-ray binary XB 1254-69 observed with XMM-Newton and INTEGRAL

M. Diaz Trigo, A. N. Parmar, L. Boirin +3

We have analysed data from five XMM-Newton observations of XB 1254-69, one of them simultaneous with INTEGRAL, to investigate the mechanism responsible for the highly variable dips…

astro-ph200651 cited

XMM-Newton and INTEGRAL spectroscopy of the microquasar GRO J1655-40 during its 2005 outburst

M. Diaz Trigo, A. N. Parmar, J. Miller +2

We report on two simultaneous XMM-Newton and INTEGRAL observations of the microquasar GRO J1655-40 during the 2005 outburst when the source was in its high-soft state. The 0.3-200…

astro-ph2005

A highly-ionized absorber as a new explanation for the spectral changes during dips from X-ray binaries

L. Boirin, M. Diaz Trigo, M. Mendez +2

Until now, the spectral changes observed from persistent to dipping intervals in dipping low-mass X-ray binaries were explained by invoking progressive and partial covering of an e…