Studying cool dwarfs and their mass function using infrared surveys
Anyone seeking to understand the physical processes of star formation must make reference to the spectrum of masses (mass function) produced by such processes. The low mass end of this mass function in particular is poorly constrained. The two leading environments in which to measure the mass functi...
| Main Author: | |
|---|---|
| Published: |
University of Edinburgh
2007
|
| Subjects: | |
| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.649266 |