arxiv: 0709.0460 · v1 · submitted 2007-09-04 · 🌌 astro-ph

Tidal tails around globular clusters

M. Montuori (1) , R. Capuzzo-Dolcetta (2) , P. Di Matteo (3) , P. Miocchi (2) ((1) CNR-INFM , Roma , Italy , (2) Dep. of Physics , La Sapienza Univ. of Roma

show 4 more authors

(3) Obs. de Paris LERMA Paris France)

This is my paper

classification 🌌 astro-ph

keywords clusterstailstidalaroundbulgeclustercomovingcoordinates

0 comments

read the original abstract

We present the results of detailed N-body simulations of clusters moving in a realistic Milky Way (MW) potential. The strong interaction with the bulge and the disk of the Galaxy leads to the formation of tidal tails, emanating from opposite sides of the cluster. Their orientation and morphology may be interpreted easily in terms of a comoving frame of coordinates.

This paper has not been read by Pith yet.

Tidal tails around globular clusters

discussion (0)