88 citations · 258 across the 9 of their papers we have counts for
26 papers · 1 filter
XMM-Newton observation of MACHO 104.20906.960: a dwarf nova candidate with a 2 h period
A. A. Nucita, S. Carpano, F. De Paolis +3
The binaries known as cataclysmic variables are particular binary systems in which the primary star (a white dwarf) accretes material from a secondary via Roche-lobe mechanism. Usu…
The globular cluster NGC 6388: -Newton and observations
A. A. Nucita, F. De Paolis, G. Ingrosso +2
By studying the optical brightness surface density of the globular cluster NGC 6388, it has been recently proposed that it harbors a central intermediate-mass black hole with mass…
Apoastron Shift Constraints on Dark Matter Distribution at the Galactic Center
A. F. Zakharov, A. A. Nucita, F. De Paolis +1
The existence of dark matter (DM) at scales of few pc down to pc around the centers of galaxies and in particular in the Galactic Center region has been considered…
Emission of gravitational waves from binary systems in the galactic center and diffraction by star clusters
P. Longo, G. Congedo, A. Nucita +2
Binary systems of compact objects are strong emitters of gravitational waves whose amplitude depends on the binary orbital parameters as the component mass, the orbital semi-major…
Solar system constraints on R gravity
A. F. Zakharov, A. A. Nucita, F. De Paolis +1
Recently, gravitational microlensing has been investigated in the framework of the weak field limit of fourth order gravity theory. However, solar system data (i.e. planetary perio…
Gravitational wave scintillation by a stellar cluster
G. Congedo, F. De Paolis, P. Longo +2
The diffraction effects on gravitational waves propagating through a stellar cluster are analyzed in the relevant approximation of Fresnel diffraction limit. We find that a gravita…