activity
20032013
most citedSimultaneous multiwavelength observations of the Low/Hard State of the X-ray transient source SWIFT J1753.5-0127

110 citations · 301 across the 11 of their papers we have counts for

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7 papers · 1 filter

astro-ph.HE2013

Comptonization in ultra-strong magnetic fields: numerical solution of the radiative transfer problem

C. Ceccobello, R. Farinelli, L. Titarchuk

We consider the radiative transfer problem in a plane-parallel slab of thermal electrons in the presence of an overcritical magnetic field. Under such conditions, the magnetic fiel…

astro-ph.HE2013★ 14 cited

The Swift Supergiant Fast X-ray Transients Project: a review, new results, and future perspectives

P. Romano, V. Mangano, L. Ducci +9

We present a review of the Supergiant Fast X-ray Transients (SFXT) Project, a systematic investigation of the properties of SFXTs with a strategy that combines Swift monitoring pro…

astro-ph.HE2013★ 46 cited

RX J0440.9+4431: a persistent Be/X-ray binary in outburst

C. Ferrigno, R. Farinelli, E. Bozzo +3

The persistent Be/X-ray binary RX J0440.9+4431 flared in 2010 and 2011 and has been followed by various X-ray facilities Swift, RXTE, XMM-Newton, and INTEGRAL. We studied the sourc…

astro-ph.HE2012

Supergiant Fast X-ray Transients with Swift: spectroscopic and temporal properties

P. Romano, V. Mangano, L. Ducci +8

Supergiant fast X-ray transients (SFXTs) are a class of high-mass X-ray binaries with possible counterparts in the high energy gamma rays. The Swift SFXT Project has conducted a sy…

astro-ph.HE2012★ 20 cited

Swift observations of two supergiant fast X-ray transient prototypes in outburst

R. Farinelli, P. Romano, V. Mangano +6

We report on the results from observations of the most recent outbursts of XTE J1739-302 and IGR J17544-2619, which are considered to be the prototypes of the supergiant fast X-ray…

astro-ph.HE2011★ 53 cited

Numerical solution of the radiative transfer equation: X-ray spectral formation from cylindrical accretion onto a magnetized neutron star

R. Farinelli, C. Ceccobello, P. Romano +1

Predicting the emerging X-ray spectra in several astrophysical objects is of great importance, in particular when the observational data are compared with theoretical models. To th…