No CrossRef data available.
Article contents
Low-metallicity Star Formation: the characteristic mass and upper mass limit
Published online by Cambridge University Press: 01 June 2008
Abstract
We consider the fragmentation mass scale of low-metallicity clouds based on their thermal evolution. Then we present the protostellar evolution in the main accretion phase, and discuss the upper limit on the stellar mass by the stellar feedback.
Keywords
- Type
- Contributed Papers
- Information
- Copyright
- Copyright © International Astronomical Union 2008