activity
19962004
most citedFormation and evolution of clumpy tidal tails around globular clusters

74 citations · 74 across the 1 of their papers we have counts for

collaborators

16 papers

astro-ph200474 cited

Formation and evolution of clumpy tidal tails around globular clusters

R. Capuzzo Dolcetta, P. Di Matteo, P. Miocchi

We present some results of numerical simulations of a globular cluster orbiting in the central region of a triaxial galaxy on a set of 'loop' orbits. Tails start forming after abou…

astro-ph2001

Large scale star formation in galaxies. II. The spirals NGC 3377A, NGC 3507 and NGC 4394

A. Vicari, P. Battinelli, R. Capuzzo--Dolcetta +2

The identification of young star groupings (YSG) in the three spiral galaxies NGC 3377A, NGC 3507, NGC 4394 is obtained by mean of the statistical method described in Paper I. We f…

astro-ph2001

An efficient parallel tree-code for the simulation of self-gravitating systems

P. Miocchi, R. Capuzzo-Dolcetta

We describe a parallel version of our tree-code for the simulation of self-gravitating systems in Astrophysics. It is based on a dynamic and adaptive method for the domain decompos…

astro-ph2001

Galactic nuclear activity induced by globular cluster merging

R. Capuzzo-Dolcetta

The interpretation of the difference observed between the radial distribution of globular clusters and that of halo-bulge stars in elliptical galaxies is discussed in terms of evol…

astro-ph2001

Application of an objective method for the identification of Young Star Groupings in spiral galaxies

R. Capuzzo-Dolcetta, A. Vicari, P. Battinelli +1

We present some results of the application of our automatic technique for the identification of Young Star Groupings (YSGs) in spiral galaxies. In this report we discuss our new re…

astro-ph2000

On the use of a heterogeneous MIMD-SIMD platform to simulate the dynamics of globular clusters with a central massive object

R. Capuzzo-Dolcetta, N. Pucello, V. Rosato +1

The dynamics of a large stellar (globular) cluster containing N=128,000 stars has been simulated by a direct summation (O(N)) method by using a heterogeneous platform. Prelimin…