activity
20172023
most citedIndications of non-conservative mass-transfer in AMXPs

30 citations · 170 across the 14 of their papers we have counts for

collaborators

18 papers

astro-ph.HE20232 cited

Low Magnetic-Field Neutron Stars in X-ray Binaries

Tiziana Di Salvo, Alessandro Papitto, Alessio Marino +2

In this chapter we give an overview of the properties of X-ray binary systems containing a weakly magnetized neutron star. These are old (Giga-years life-time) semi-detached binary…

astro-ph.HE20228 cited

Investigating the nature and properties of MAXI J1810-222 with radio and X-ray observations

T. D. Russell, M. Del Santo, A. Marino +10

We present results from radio and X-ray observations of the X-ray transient MAXI J1810-222. The nature of the accretor in this source has not been identified. In this paper, we sho…

astro-ph.HE202210 cited

Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925

Chiara Salvaggio, Anna Wolter, Fabio Pintore +7

Variability is a powerful tool to investigate properties of X-ray binaries (XRB), in particular for Ultraluminous X-ray sources (ULXs) that are mainly detected in the X-ray band. F…

astro-ph.HE202115 cited

Spectral analysis of the low-mass X-ray pulsar 4U 1822-371: Reflection component in a high-inclination system

A. Anitra, T. Di Salvo, R. Iaria +6

The X-ray source 4U 1822-371 is an eclipsing low-mass X-ray binary and X-ray pulsar, hosting a NS that shows periodic pulsations in the X-ray band. The inclination angle of the sys…

astro-ph.HE20218 cited

Fe K and Fe K line detection in the NuSTAR spectrum of the ultra-bright Z-source Scorpius X-1

S. M. Mazzola, R. Iaria, T. Di Salvo +8

Low-mass X-ray binaries hosting a low-magnetised neutron star, which accretes matter via Roche-lobe overflow, are generally grouped in two classes, named Atoll and Z sources after…

astro-ph.HE202012 cited

Evidence of a non-conservative mass transfer in the ultra-compact X-ray source XB 1916-053

R. Iaria, A. Sanna, T. Di Salvo +5

The dipping source XB 1916-053 is a compact binary system with an orbital period of 50 min harboring a neutron star. Using ten new {\it Chandra} observations and one {\it Swift/XRT…