arXiv Analytics

Sign in

arXiv:1111.0294 [astro-ph.GA]AbstractReferencesReviewsResources

Do all O stars form in star clusters?

Carsten Weidner, Vasilii V. Gvaramadze, Pavel Kroupa, Jan Pflamm-Altenburg

Published 2011-11-01Version 1

The question whether or not massive stars can form in isolation or only in star clusters is of great importance for the theory of (massive) star-formation as well as for the stellar initial mass function of whole galaxies (IGIMF-theory). While a seemingly easy question it is rather difficult to answer. Several physical processes (e.g. star-loss due to stellar dynamics or gas expulsion) and observational limitations (e.g. dust obscuration of young clusters, resolution) pose severe challenges to answer this question. In this contribution we will present the current arguments in favour and against the idea that all O stars form in clusters.

Comments: 6 pages, 3 Figures, to appear in the proceedings of "Stellar Clusters and Associations - A RIA workshop on GAIA", 23-27 May 2011, Granada, Spain
Categories: astro-ph.GA, astro-ph.SR
Related articles: Most relevant | Search more
arXiv:1011.1905 [astro-ph.GA] (Published 2010-11-08)
The galaxy-wide IMF - from star clusters to galaxies
arXiv:1812.01615 [astro-ph.GA] (Published 2018-12-04)
Star Clusters Across Cosmic Time
arXiv:0910.4579 [astro-ph.GA] (Published 2009-10-24)
The evolution of the stellar mass function in star clusters