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Conference object . 2019
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Conference object . 2019
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Other literature type . 2019
License: CC BY
Data sources: ZENODO
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Star formation efficiency of magnetized, turbulent and rotating molecular cloud above the critical mass

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 30 Nov 2019 English Publisher:Zenodo
Authors: Gemechu M. Kumssa; S. B. Tessema;

doi: 10.5281/zenodo.3558434 , 10.5281/zenodo.3558435

Star formation efficiency of magnetized, turbulent and rotating molecular cloud above the critical mass

Abstract

The formation of stars constitutes one of the basic problems of astrophysics. Understanding of star formation efficiency of molecular clouds (MCs) of a galaxy is necessary for studying the galactic evolution. Present data and theoretical formulations show that the structure and dynamics of the Galactic interstellar medium (ISM) are extremely complex. So that there is no simple model that can explain adequately the star formation efficiency of MCs because of its perplexing nature. The initial mass of the cloud needed for collapse varies based on the environment in which the cloud resides and the strength of its magnetic field, turbulence as well as the speed of rotation. In this paper, we estimate the star formation efficiency by combining predetermined models and the critical mass formulated by Kumssa and Tessema (2018).

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Keywords

Star, SFE, Critical mass

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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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