The existence of dark matter at scales of a few parsecs down to 10^-5 pc at the center of the Galaxy has been considered in the literature. Under the assumption that a dark matter clump exists, the study of the gamma-ray emission from the galactic center allows us to constraint both the mass and the size of this distribution. Here we also discuss the constraints coming from the analysis of the S2 and S16 stars orbiting around SgrA*
We describe a universal profile of dark matter particles in the inner parsec of the Galaxy, rho ~ r^...
We investigate constraints on the distribution of dark matter in the neighbourhood of the Galactic c...
In this work we characterize the distribution of Dark Matter (DM) in the Milky Way (MW), and its unc...
The existence of dark matter (DM) at scales of a few parsecs down to similar or equal to 10(-5) pc a...
The existence of dark matter (DM) at scales of few pc down to similar or equal to 10(-5) pc around t...
The existence of dark matter (DM) at scales of few pc down to ~ 10-5 pc around the centers of galaxi...
In this work I use astrometric and spectroscopic data on the S2 star at the Galactic centre (GC) up ...
A concept of dark matter (DM) is introduced. As for other anomalies, we describe two ways to solve ...
We have recently introduced a new model for the distribution of dark matter (DM) in galaxies based o...
We discuss constraints on the properties and nature of the dark mass concentration at the core of th...
Several stars orbit the - 3.67 x 10(6) M-circle dot black hole in the center of our Galaxy. Predicti...
An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data...
We derive constraints on parameters of generic dark matter candidates by comparing the-oretical pred...
An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data...
Journal ArticleDark matter annihilation has been proposed to explain the TeV gamma rays observed fro...
We describe a universal profile of dark matter particles in the inner parsec of the Galaxy, rho ~ r^...
We investigate constraints on the distribution of dark matter in the neighbourhood of the Galactic c...
In this work we characterize the distribution of Dark Matter (DM) in the Milky Way (MW), and its unc...
The existence of dark matter (DM) at scales of a few parsecs down to similar or equal to 10(-5) pc a...
The existence of dark matter (DM) at scales of few pc down to similar or equal to 10(-5) pc around t...
The existence of dark matter (DM) at scales of few pc down to ~ 10-5 pc around the centers of galaxi...
In this work I use astrometric and spectroscopic data on the S2 star at the Galactic centre (GC) up ...
A concept of dark matter (DM) is introduced. As for other anomalies, we describe two ways to solve ...
We have recently introduced a new model for the distribution of dark matter (DM) in galaxies based o...
We discuss constraints on the properties and nature of the dark mass concentration at the core of th...
Several stars orbit the - 3.67 x 10(6) M-circle dot black hole in the center of our Galaxy. Predicti...
An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data...
We derive constraints on parameters of generic dark matter candidates by comparing the-oretical pred...
An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data...
Journal ArticleDark matter annihilation has been proposed to explain the TeV gamma rays observed fro...
We describe a universal profile of dark matter particles in the inner parsec of the Galaxy, rho ~ r^...
We investigate constraints on the distribution of dark matter in the neighbourhood of the Galactic c...
In this work we characterize the distribution of Dark Matter (DM) in the Milky Way (MW), and its unc...