2 citations · 2 across the 3 of their papers we have counts for
3 papers
astro-ph2004
How star clusters could survive low star formation efficiencies
M. Fellhauer, P. Kroupa
After the stars of a new, embedded star cluster have formed they blow the remaining gas out of the cluster. Especially winds of high mass stars and definitely the on-set of the fir…
astro-ph2004
A Formation Scenario for the Heavy-Weight Cluster W3 in NGC 7252
M. Fellhauer, P. Kroupa
The young star cluster W3 (age 300-500 Myr) in NGC 7252 is the most luminous star cluster known to date. Dynamical mass estimates result in 8 +/- 2 * 10^7 M_sun. With an effective…
astro-ph2004★ 2 cited
omega-Centauri - an Ultra Compact Dwarf Galaxy ?
M. Fellhauer
A new formation scenario for omega-Cen is presented, in which omega-Cen has formed from a star cluster complex (= super-cluster). The star-burst which has led to the formation of t…