Star Formation in Self-Gravitating Molecular Cloud: The Critical Mass and the Core Accretion Rate

Journals Menu

Follow SCIRP

ISSN Print: 2160-049X
ISSN Online: 2160-0503
www.scirp.org/journal/wjm
E-mail: wjm@scirp.org

"Star Formation in Self-Gravitating Molecular Cloud: The Critical Mass and the Core Accretion Rate"
written by Gemechu M. Kumssa, S. B. Tessema,
published by World Journal of Mechanics, Vol.10 No.5, 2020

has been cited by the following article(s):

[1]	The role of thermodynamic efficiency in setting the star formation efficiency of self‐gravitating molecular clouds
	2020

Follow SCIRP

[1]	The role of thermodynamic efficiency in setting the star formation efficiency of self‐gravitating molecular clouds Astronomische Nachrichten, 2020 DOI:10.1002/asna.202013807

[2]	The role of thermodynamic efficiency in setting the star formation efficiency of self‐gravitating molecular clouds Astronomische Nachrichten, 2020 DOI:10.1002/asna.202013807