activity
20052026
most citedSwings between rotation and accretion power in a millisecond binary pulsar

460 citations · 3k across the 103 of their papers we have counts for

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Showing 2015 · astro-ph.HEShow all

5 papers · 2 filters

astro-ph.HE2015★ 21 cited

SAX J1808.4-3658, an accreting millisecond pulsar shining in gamma rays?

E. de Ona Wilhelmi, A. Papitto, J. Li +7

We report the detection of a possible gamma-ray counterpart of the accreting millisecond pulsar SAX J1808.4-3658. The analysis of ~6 years of data from the Large Area Telescope on…

astro-ph.HE2015★ 22 cited

Signature of the presence of a third body orbiting around XB 1916-053

R. Iaria, T. Di Salvo, A. F. Gambino +9

The ultra-compact dipping source \object{XB 1916-053} has an orbital period of close to 50 min and a companion star with a very low mass (less than 0.1 M). The orbital pe…

astro-ph.HE2015★ 36 cited

Study of the reflection spectrum of the accreting neutron star GX 3+1 using XMM-Newton and INTEGRAL

Fabio Pintore, Tiziana Di Salvo, Enrico Bozzo +6

Broad emission features of abundant chemical elements, such as Iron, are commonly seen in the X-ray spectra of accreting compact objects and their studies can provide useful inform…

astro-ph.HE2015★ 26 cited

A possible cyclotron resonance scattering feature near 0.7 keV in X1822-371

R. Iaria, T. Di Salvo, M. Matranga +9

We analyse all available X-ray observations of X1822-371 made with XMM-Newton, Chandra, Suzaku and INTEGRAL satellites. The observations were not simultaneous. The Suzaku and INTEG…

astro-ph.HE2015★ 54 cited

Suzaku broad-band spectrum of 4U 1705-44: Probing the Reflection component in the hard state

T. Di Salvo, R. Iaria, M. Matranga +7

Iron emission lines at 6.4-6.97 keV, identified with Kalpha radiative transitions, are among the strongest discrete features in the X-ray band. These are one of the most powerful p…