activity
19982009
most citedNear-IR properties of 24 Globular Clusters in the Galactic Bulge

177 citations · 1.8k across the 30 of their papers we have counts for

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Showing 2003Show all

11 papers · 1 filter

astro-ph2003

The chemical composition of the peculiar companion to the millisecond pulsar in NGC 6397

E. Sabbi, R. G. Gratton, A. Bragaglia +4

We present the chemical composition of the bright companion to the millisecond pulsar J1740-5340 in NGC 6397, based on high resolution spectra. Though the large rotation velocity o…

astro-ph2003

The Helium White Dwarf orbiting the Millisecond Pulsar in the halo of the Globular Cluster NGC 6752

Francesco R. Ferraro, Andrea Possenti, Elena Sabbi +1

We have used deep high-resolution multiband images taken at the ESO Very Large Telescope to identify the optical binary companion to the millisecond pulsar (PSR J1911-5958A) locate…

astro-ph2003

The Nuclear Structure of the Sagittarius Dwarf Spheroidal Galaxy

Lorenzo Monaco, Michele Bellazzini, Francesco R. Ferraro +1

We present a study of the central parts of the Sagittarius dwarf spheroidal galaxy (Sgr). We found a clear overdensity of Sgr's stars around M~54 (hereafter NS). NS is well represe…

astro-ph2003

Blue Horizontal Branch Stars in the Sagittarius dwarf spheroidal galaxy

Lorenzo Monaco, Michele Bellazzini, Francesco R. Ferraro +1

We report on the recovery of a Blue Horizontal Branch (BHB) population belonging to the Sagittarius Dwarf Spheroidal Galaxy (Sgr). The sequence is clearly identified in the (V, V-I…

astro-ph20031 cited

Globular Clusters in the Sgr Stream and other structures

M. Bellazzini, R. Ibata, F. R Ferraro

The possible association of Galactic globular clusters with the Sgr Stream is shortly reviewed at the light of the most recent observations of the Stream. >= 20 % of the Galactic g…

astro-ph2003

The puzzling dynamical status of the core of the globular cluster NGC 6752

F. R. Ferraro, A. Possenti, E. Sabbi +4

We have used high resolution WFPC2-HST and ground based Wide Field images to determine the center of gravity and construct an extended radial density and brightness profile of the…