How did globular clusters lose their gas?

Autor:	Charbonnel, C., Krause, M., Decressin, T., Meynet, G., Prantzos, N., Diehl, R.
Rok vydání:	2012
Předmět:	Astrophysics - Galaxy Astrophysics
Druh dokumentu:	Working Paper
Popis:	We summarize the results presented in Krause et al. (2012) on the impact of supernova-driven shells and dark-remnant accretion on gas expulsion in globular cluster infancy. Comment: 2 pages, 2 figures; Invited talk presented at Special Session 1 "Origin and Complexity of Massive Star Clusters" at IAU General Assembly XXVIII, Beijing 2012. To appear in Highlights of Astronomy
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/1211.0143 Zobrazit plný text záznamu View this record from Arxiv