Details

Autor(en) / Beteiligte

• Shukirgaliyev, Bekdaulet
• Parmentier, Genevieve
• Berczik, Peter
• Just, Andreas

Titel

Star Clusters in the Galactic tidal field, from birth to dissolution

Ist Teil von

• Proceedings of the International Astronomical Union, 2019-05, Vol.14 (S351), p.507-511

Ort / Verlag

Cambridge: Cambridge University Press

Erscheinungsjahr

2019

Link zum Volltext

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• Abstract We study the evolution of star clusters in the Galactic tidal field starting from their birth in molecular clumps. Our model clusters form according to the local-density-driven cluster formation model in which the stellar density profile is steeper than that of gas. As a result, clusters resist the gas expulsion better than predicted by earlier models. We vary the impact of the Galactic tidal field λ , considering different Galactocentric distances (3-18 kpc), as well as different cluster sizes. Our model clusters survive the gas expulsion independent of λ . We investigated the relation between the cluster mass at the onset of secular evolution and their dissolution time. The model clusters formed with a high star-formation efficiency (SFE) follow a tight mass-dependent dissolution relation, in agreement with previous theoretical studies. However, the low-SFE models present a shallower mass-dependent relation than high-SFE clusters, and most dissolve before reaching 1 Gyr (cluster teenage mortality).