Luigi Stella

TL;DR: In this paper, the results of the XMM-Newton observations of five hard X-ray emitters: IGR J08262-3736 (IGR J17354-3255), IGRJ16328-4726, SAX J1818.6-1703, and IGR j17348-2045 (IGR J17342045) were presented.

TL;DR: In this paper, the steady state pulsar X-ray luminosity distribution as a function of the star formation rate (SFR) in the galaxy is estimated, and it is shown that a few percent of galaxies are dominated by a single bright pulsar with LX 1039 ergs s-1, roughly independently of its SFR.

TL;DR: In this paper, the authors discovered 8.9s X-ray pulsations in 2E0050.1-7247 in the Small Magellanic Cloud (SMC) and revealed a pronounced Halpha activity from at least two B stars in the error circles.

TL;DR: In this paper, the authors reported on the first dedicated monitoring campaign of the source in the soft X-ray range with XMM-Newton and Swift/XRT, which confirmed the association of XTEJ1743-363 with the previously suggested M8 III giant and the classification of the sources as a member of the Symbiotic X-rays binaries.

TL;DR: In this paper, the long-term spectral and timing characteristics of SGR 1833-0832 were studied, which span about 225 days, and it was shown that the source X-ray spectrum is well described by an absorbed blackbody, with temperature kT=1.2 keV and absorbing column nH=(10.4+/-0.2)E22 cm^-2.