Astrophysics (index)

Dense Core

(Core)
(dense molecular cloud)

The term Dense Core (in discussions of Star Formation (SF)) to refer to a dense Molecular Cloud or a dense region of a molecular cloud, which would be a necessary stage in the development of stars from clouds. Current star formation models theorize them, and apparent examples are observed, e.g., in well-known clouds in Orion. The term refers to a mass of Hydrogen (H) that is gravitationally bound or very close to that state, i.e., a Jeans Length is established.

A Coherent Dense Core is such a region that is relatively calm, i.e., has thermal Kinetic Energy but lacks the degree of Turbulence evident in the region around it. Current research aims to understand their formation and evolution into stars.

As far as I can tell, in the context of star formation, the word Core (without the word "dense") can refer to a dense core, or (by context) can refer to the core of a subsequent Protostar.


(hydrogen,star formation,clouds,molecular hydrogen,gas)
http://en.wikipedia.org/wiki/Protostar
http://arxiv.org/abs/1602.00707

Referenced by:
COMPLETE Survey
Dense Core Mass Function (DCMF)
Dendrogram
Filament
Infrared Dark Cloud (IRDC)
LDN 1689
Mach Number
Virial Parameter

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