Formation and Properties of Molecular Cloud Cores

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Paper of invited talk at the 2008 french astronomical society meeting (SF2A-2008). 4 pages; 4 figures. A few typos corrected i

Scientific paper

In this paper, we review some of the properties of dense molecular cloud cores. The results presented here rely on three-dimensional numerical simulations of isothermal, magnetized, turbulent, and self-gravitating molecular clouds (MCs) in which dense core form as a consequence of the gravo-turbulent fragmentation of the clouds. In particular we discuss issues related to the mass spectrum of the cores, their lifetimes and their virial balance.

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