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20002026
most citedSwings between rotation and accretion power in a millisecond binary pulsar

460 citations · 1.8k across the 43 of their papers we have counts for

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Showing 2010Show all

5 papers · 1 filter

astro-ph.IM2010★ 13 cited

LOFT - a Large Observatory For x-ray Timing

M. Feroci, L. Stella, A. Vacchi +46

The high time resolution observations of the X-ray sky hold the key to a number of diagnostics of fundamental physics, some of which are unaccessible to other types of investigatio…

astro-ph.HE2010★ 55 cited

New ephemeris of the ADC source 2A 1822-371: a stable orbital-period derivative over 30 years

L. Burderi, T. Di Salvo, A. Riggio +4

We report on a timing of the eclipse arrival times of the low mass X-ray binary and X-ray pulsar 2A 1822-371 performed using all available observations of the Proportional Counter…

astro-ph.HE2010★ 50 cited

Spin down during quiescence of the fastest known accretion-powered pulsar

A. Papitto, A. Riggio, L. Burderi +3

We present a timing solution for the 598.89 Hz accreting millisecond pulsar, IGR J00291+5934, using Rossi X-ray Timing Explorer data taken during the two outbursts exhibited by the…

astro-ph.HE2010★ 73 cited

The X-ray spectrum of the newly discovered accreting millisecond pulsar IGR J17511-3057

A. Papitto, A. Riggio, T. Di Salvo +5

We report on an XMM-Newton observation of the accreting millisecond pulsar, IGR J17511-3057. Pulsations at 244.8339512(1) Hz are observed with an RMS pulsed fraction of 14.4(3)%. A…

astro-ph.HE2010★ 60 cited

A self-consistent approach to the hard and soft states of 4U 1705-44

A. D'Aì, T. Di Salvo, D. Ballantyne +10

We analyzed two XMM-Newton observations of the bright atoll source 4U 1705-44, which can be considered a prototype of the class of the persistent NS LMXBs showing both hard and sof…