Publication not explained
This publication has not yet been explained in plain language by the author(s). However, you can still read the publication.
If you are one of the authors, claim this publication so you can create a plain language summary to help more people find, understand and use it.
Featured Image
Read the Original
This page is a summary of: Present-day star formation: From molecular cloud cores to protostars and protoplanetary disks, Progress of Theoretical and Experimental Physics, January 2012, Oxford University Press (OUP),
DOI: 10.1093/ptep/pts024.
You can read the full text:
Contributors
The following have contributed to this page