activity
20072016
most citedA new model for the X-ray continuum of the magnetized accreting pulsars

64 citations · 202 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2016★ 21 cited

Swift J174540.7-290015: a new accreting binary in the Galactic Center

G. Ponti, C. Jin, B. De Marco +8

We report on the identification of the new Galactic Center (GC) transient Swift J174540.7-290015 as a likely low mass X-ray binary (LMXB) located at only 16 arcsec from Sgr A*. Thi…

astro-ph.HE2016★ 39 cited

Clumpy wind accretion in supergiant neutron star high mass X-ray binaries

E. Bozzo, L. Oskinova, A. Feldmeier +1

The accretion of the stellar wind material by a compact object represents the main mechanism powering the X-ray emission in classical supergiant high mass X-ray binaries and superg…

astro-ph.HE2016★ 17 cited

IGR J17451-3022: a dipping and eclipsing low mass X-ray binary

E. Bozzo, P. Pjanka, P. Romano +10

In this paper, we report on the available X-ray data collected by INTEGRAL, Swift, and XMM-Newton during the first outburst of the INTEGRAL transient IGR J17451-3022, discovered in…

astro-ph.HE2016★ 64 cited

A new model for the X-ray continuum of the magnetized accreting pulsars

R. Farinelli, C. Ferrigno, E. Bozzo +1

Accreting highly magnetized pulsars in binary systems are among the brightest X-ray emitters in our Galaxy. Although a number of high statistical quality broad-band (0.1-100 keV) X…

astro-ph.HE2010★ 47 cited

Spectral and timing properties of the accreting X-ray millisecond pulsar IGR J17511-3057

M. Falanga, L. Kuiper, J. Poutanen +6

IGR J17511-3057 is the second X-ray transient accreting millisecond pulsar discovered by INTEGRAL. It was in outburst for about a month from September 13, 2009. The broad-band aver…

astro-ph2007★ 14 cited

X-Ray Eclipse Time Delays in 4U2129+47

E. Bozzo, M. Falanga, A. Papitto +8

4U 2129+47 was discovered in the early 80's and classified as an accretion disk corona source due to its broad and partial X-ray eclipses. The 5.24 hr binary orbital period was inf…