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

collaborators
Showing 2017Show all

7 papers · 1 filter

astro-ph.HE2017★ 54 cited

Discovery of 105 Hz coherent pulsations in the ultracompact binary IGR J16597-3704

A. Sanna, A. Bahramian, E. Bozzo +15

We report the discovery of X-ray pulsations at 105.2 Hz (9.5 ms) from the transient X-ray binary IGR J16597-3704 using NuSTAR and Swift. The source was discovered by INTEGRAL in th…

astro-ph.HE2017★ 13 cited

Evidence of a non-conservative mass transfer for XTE J0929-314

A. Marino, T. Di Salvo, A. F. Gambino +5

Context. In 1998 the first accreting millisecond pulsar, SAX J1808.4-3658, was discovered and to date 18 systems showing coherent, high frequency (> 100 Hz) pulsations in low mass…

astro-ph.HE2017★ 5 cited

Updating the orbital ephemeris of the dipping source XB 1254-690 and the distance to the source

A. F. Gambino, R. Iaria, T. Di Salvo +5

XB 1254-690 is a dipping low mass X-ray binary system hosting a neutron star and showing type I X-ray bursts. We aim at obtaining more accurate orbital ephemeris and at constrainin…

astro-ph.HE2017★ 47 cited

On the timing properties of SAX J1808.4-3658 during its 2015 outburst

A. Sanna, T. Di Salvo, L. Burderi +7

We present a timing analysis of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1808.4-3658, using non-simultaneous XMM-Newton and NuStar observations. We estimate…

astro-ph.HE2017★ 21 cited

Study of the accretion torque during the 2014 outburst of the X-ray pulsar GRO J1744-28

A. Sanna, A. Riggio, L. Burderi +9

We present the spectral and timing analysis of the X-ray pulsar GRO J1744-28 during its 2014 outburst using data collected with the X-ray satellites Swift, INTEGRAL, Chandra, and X…

astro-ph.HE2017★ 29 cited

A possible solution of the puzzling variation of the orbital period of MXB 1659-298

R. Iaria, A. F. Gambino, T. Di Salvo +6

MXB 1659-298 is a transient neutron star Low-Mass X-ray binary system that shows eclipses with a periodicity of 7.1 hr. The source went to outburst in August 2015 after 14 years of…