activity
20002015
most citedOn the Nature of Feedback Heating in Cooling Flow Clusters

221 citations · 834 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.HE2015★ 29 cited

NGC 2276: a remarkable galaxy with a large number of ULXs

Anna Wolter, Paolo Esposito, Michela Mapelli +2

The starbusting, nearby (D = 32.9 Mpc) spiral (Sc) galaxy NGC2276 belongs to the sparse group dominated by the elliptical galaxy NGC2300. NGC2276 is a remarkable galaxy, as it disp…

astro-ph.HE2012★ 46 cited

PSR J0357+3205: the tail of the turtle

Martino Marelli, Andrea De Luca, David Salvetti +6

Using a new XMM-Newton observation, we have characterized the X-ray properties of the middle-aged radio-quiet gamma-ray pulsar J0357+3205 (named Morla) and its tail. The X-ray emis…

astro-ph.HE2012

Stochastic accretion and the variability of supergiant fast X-ray transients

Fabio Pizzolato, Lara Sidoli

In this paper we consider the variability of the luminosity of a compact object (CO) powered by the accretion of an extremely inhomogeneous ("clumpy") stream of matter. The accreti…

astro-ph.HE2011★ 20 cited

A time-variable, phase-dependent emission line in the X-ray spectrum of the isolated neutron star RX J0822-4300

A. De Luca, D. Salvetti, A. Sartori +9

RX J0822-4300 is the Central Compact Object associated with the Puppis A supernova remnant. Previous X-ray observations suggested RX J0822-4300 to be a young neutron star with a we…

astro-ph.HE2011★ 29 cited

The XMM-Newton view of Supergiant Fast X-ray Transients: the case of IGRJ16418-4532

L. Sidoli, S. Mereghetti, V. Sguera +1

We report on a 40 ks long, uninterrupted X-ray observation of the candidate supergiant fast X-ray transient (SFXT) IGRJ16418-4532 performed with XMM-Newton on February 23, 2011. Th…

astro-ph.HE2011★ 58 cited

X-ray and optical observations of the unique binary system HD49798/RXJ0648.0-4418

S. Mereghetti, N. La Palombara, A. Tiengo +5

We report the results of XMM-Newton observations of HD49798/RXJ0648.0-4418, the only known X-ray binary consisting of a hot sub-dwarf and a white dwarf. The white dwarf rotates ver…